The galaxy presents as a moderately luminous, elliptical system with a smooth, centrally concentrated morphology. Its overall color profile suggests an older stellar population, indicated by the yellowish hue dominating the core and extending into the surrounding halo. There is a notable absence of distinct spiral arm structures or prominent dust lanes, reinforcing the classification as an elliptical galaxy. The galaxy exhibits a slight elongation, deviating marginally from a perfectly circular shape. No signs of significant tidal disturbances or ongoing merger activity are immediately apparent, although subtle asymmetries within the extended halo cannot be definitively ruled out without further analysis. The galaxy's light is fairly compact, suggesting a relatively high density of stars within its effective radius.
