The galaxy presents a generally elliptical morphology, though with some notable deviations from a perfectly smooth profile. A dominant central bulge exhibits a yellowish-orange hue, indicative of an older stellar population. Fainter, bluer regions are visible extending from either side of this bulge.

The galaxy shows evidence of an ongoing or recent interaction or merger. The isophotes are somewhat disturbed, and there appear to be asymmetrical extensions emanating from the main body. The presence of bluer regions suggests areas of more active star formation, possibly triggered by the interaction. There may be a faint tidal tail or stream visible on one side of the galaxy.
