The galaxy appears to be a relatively compact, elliptical type, characterized by a smooth, centrally concentrated light distribution. It presents a generally round morphology, with only a slight deviation towards a more elongated shape. The core region exhibits a bright, intense yellow-white hue, indicative of an older stellar population. There is subtle evidence of bluer, more diffuse light surrounding the central bulge, hinting at some recent, but low level, star formation activity in the outer regions. There is no clear indication of strong spiral arm structures or major disturbances from interactions. Subtle asymmetries might point towards a minor merging event in its past, but its current form is generally relaxed and undisturbed.
