The galaxy exhibits a generally elliptical morphology, though there is an indication of interaction or disturbance. One can see a fairly prominent central bulge, appearing smooth in texture, with a concentrated yellowish color. To one side of the central bulge, there is a separate region of diffuse, bluish-pink emission, indicative of on-going star formation, likely induced by the interaction. The primary body of the galaxy, particularly the central bulge, is significantly brighter than the disturbed region. There is no clear spiral arm structure, instead an overall amorphous appearance suggestive of a post-merger state or ongoing tidal disruption.
