The galaxy presents an overall smooth morphology, with a dominant, concentrated central bulge. The galaxy exhibits an elliptical shape, appearing more elongated than perfectly spherical. A subtle disk structure might be present, but is not well defined due to the smooth appearance. Color gradients within the galaxy suggest the presence of differing stellar populations. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy display bluer tones, which may be due to more recent star formation events in these regions. There is little evidence of spiral arms or significant dust lanes. No strong tidal features or signs of major mergers are apparent, although there are subtle asymmetries in the outer halo of the galaxy which could suggest a minor interaction in the past. 
