The galaxy presents as an elongated, elliptical form. The central region displays a concentrated luminosity, suggesting a significant density of stars. The color profile is dominated by warmer tones, trending towards yellow and red, indicative of an older stellar population with suppressed ongoing star formation. There is a noticeable absence of distinct spiral arm structures or prominent dust lanes. The outer regions appear diffuse, lacking sharp boundaries, and fading into the background sky. No signs of a major merger event or significant tidal disturbances are apparent. The smooth, regular morphology suggests a relatively quiescent evolutionary state.
