The galaxy presents an elliptical morphology, with a smooth and concentrated light distribution. The core is characterized by a bright, yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation. The outer regions exhibit a gradual decrease in luminosity, fading into a more reddish color, which could indicate a lower density of stars or a slightly older age of the stars in these regions. The overall shape appears mostly spheroidal with a slight elongation that could indicate a degree of rotation or tidal interaction in the past. No prominent dust lanes or spiral arm structures are discernible. Based on the smooth, featureless appearance and color profile, the galaxy is likely an evolved system that is not currently undergoing rapid star formation. There is no evidence of any significant recent merger or major disturbances in its morphology.
