The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish-white hue, indicative of an older stellar population. The isophotes are generally regular and lack significant deviations, suggesting a relaxed dynamical state. There is minimal evidence of spiral arm structures or dust lanes. The outer regions of the galaxy display a gradual decline in surface brightness, transitioning into a diffuse halo. The color gradient transitions to a redder hue in the halo, indicating a potential shift in stellar population composition compared to the central bulge. There appear to be no ongoing major mergers or significant tidal disturbances detected in this image. There may be a close companion. 
