The galaxy presents as a centrally concentrated object with a smooth overall appearance, suggestive of an elliptical morphology. The light distribution is relatively uniform, lacking prominent spiral arms or distinct features like dust lanes. The color profile transitions from a warmer, yellower hue at the core to slightly cooler, redder tones in the outer regions. This could indicate an older stellar population dominating the central region with a gradual decrease in age towards the outskirts. There is a noticeable absence of significant blue light, which implies a lack of ongoing, substantial star formation. The galaxy's shape appears close to circular. Overall, this galaxy exhibits characteristics consistent with a relatively massive, passively evolving system.
