The galaxy presents as a relatively smooth and rounded object, exhibiting characteristics consistent with an elliptical morphology. There's a slight color gradient observable from the center outwards with the outer regions displaying a bluer hue, suggestive of a moderate presence of younger stellar populations, although the overall color suggests a dominance of older, redder stars. There's minimal evidence of spiral arms or a distinct disk structure. Some minor disturbances may be present around the galaxy but do not seem to drastically affect the galaxy's overall morphology. The galaxy appears to be relatively isolated within its immediate field, with no clear signs of ongoing mergers or significant tidal interactions with neighboring galaxies.
