The galaxy presents as a centrally concentrated elliptical or lenticular structure. It exhibits a relatively smooth morphology, lacking prominent spiral arms or significant dust lanes. The core region displays a bright, concentrated luminosity, suggesting a high density of stars. The color profile indicates a generally redder hue, implying an older stellar population and lower ongoing star formation activity. There are faint signs of a possible extended halo or diffuse outer region, but the signal is weak. The galaxy's shape is close to but not completely circular. There is no obvious interaction or signs of any tidal disruption.