The galaxy presents an overall smooth morphology, although subtle features are discernible. The light distribution suggests two primary components: a brighter, more concentrated core and a fainter, elongated extension.

The core exhibits a near-spherical shape and emits a predominantly bluish-green hue. This coloration suggests the presence of relatively young, hot stars or significant ionized gas emission.

Extending from this central region is a more elongated structure. Its light appears redder in comparison to the core, potentially indicating an older stellar population or increased dust obscuration. The elongation is somewhat irregular in form, suggesting a possible tidal disturbance or ongoing interaction.

While the primary structure appears as a single object, faint wisps or extensions are observed hinting at the possibility of a minor merger or internal disruption. The overall structure suggests a possible intermediate stage between an elliptical and a disturbed spiral, with the central bulge dominating.
