The galaxy presents an overall smooth morphology with a noticeable elliptical shape. Its color profile exhibits a central concentration of yellowish light, suggestive of an older stellar population. There is evidence of a faint, diffuse disk surrounding the central bulge. The galaxy appears to be undergoing some form of interaction or disturbance, seen most clearly by a small, blue companion object that may either be a star-forming region or another galaxy in the process of merging. Overall, this galaxy doesn't show any strong spiral arm structures or signs of extensive star formation throughout, apart from the blue region.