The galaxy presents as a somewhat diffuse object with a moderate degree of central concentration. It displays a disturbed morphology, possibly indicative of an ongoing or recent interaction or merger event. The light distribution is not entirely smooth, showing irregularities that may be tidal features or remnants of interacting galaxies.

The central region exhibits a yellowish-white hue, suggesting an older stellar population or significant dust obscuration. There appears to be a more extended, fainter component with a reddish tint, possibly indicating the presence of dust lanes or regions of active star formation.

The overall shape is somewhat elliptical, but with noticeable deviations from perfect symmetry. There is evidence of a possible secondary core or tidal tail extending from the main body of the galaxy, further supporting the hypothesis of a past or present interaction.
