This galaxy exhibits a generally elliptical morphology, presenting a smooth, though slightly disturbed, structure. A concentrated central bulge is apparent, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter, bluer light extends outwards from the bulge along the major axis, potentially indicative of ongoing star formation within a disk or extended structure. There are hints of some tidal disturbances. The overall impression is that of a galaxy undergoing some form of interaction or internal transformation, possibly a minor merger event, with star formation.
