The galaxy presents as a roughly elliptical form, appearing elongated but with a relatively smooth overall structure. The core region exhibits a high degree of central concentration, with a bright, almost unresolved appearance. Moving outward from the core, the luminosity gradually decreases, indicating a diffuse outer halo. There are subtle variations in color across the galaxy's body, with a slightly yellower or redder hue dominating the central regions, suggestive of an older stellar population. The outer regions appear marginally bluer, possibly indicating the presence of younger, hotter stars, or potentially subtle evidence of low-level star formation activity. The galaxy shows no readily apparent spiral arm structures or prominent dust lanes, further supporting its classification as an elliptical or lenticular galaxy. There are some possible minor disturbances but the galaxy's overall smooth morphology indicates little major merger activity recently.
