The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its color suggests an older stellar population, with a yellowish-orange hue dominating the central region and extending into the surrounding halo. There is a faint, diffuse halo surrounding the main body of the galaxy, suggesting a gradual decrease in stellar density with increasing distance from the center. The galaxy exhibits a slight elongation, possibly indicating an E4 or E5 classification on the Hubble sequence. There are no prominent dust lanes or spiral arm structures visible. The smooth morphology indicates a lack of significant recent star formation. There may be slight indication of tidal disruption, however, there is no merger happening with this galaxy in it's current state. 
