This galaxy exhibits a complex morphological structure. It appears to consist of at least two distinct luminous components, suggesting a possible interaction or recent merger event. One component presents a bluer hue, indicative of ongoing star formation, while the other has a redder appearance, implying an older stellar population.

There is some evidence of possible tidal features or minor disturbances, indicating gravitational interactions. The galaxy is not uniformly smooth, but it is also not intensely disturbed, suggestive of a relatively early stage in a merger or interaction. The overall shape is somewhat irregular, lacking a clear spiral or elliptical form.

The galaxy possesses a moderate level of star formation.
