The galaxy presents a complex morphology, appearing to be in a state of interaction or recent merger. A bright, somewhat compact core region dominates the visual impression. This central region exhibits a bluish-white hue, suggestive of active star formation and the presence of hot, young stars.

Extending away from this central core is a fainter, more diffuse structure, elongated in one direction. This extension displays a redder color gradient compared to the core, which could indicate an older stellar population, dust obscuration, or a combination of both. The overall shape of this extended feature is irregular, indicating a disruption of a more ordered morphology.

There are hints of tidal features or streams emanating from the galaxy, reinforcing the hypothesis of an ongoing or recent interaction. These features are faint and somewhat indistinct.

The presence of both a bright, blue core and an extended, redder structure implies a complex star formation history and dynamic interplay of gravitational forces. Higher resolution imaging and spectroscopic data would be required to fully unravel the details of the galaxy's evolutionary state.
