The galaxy presents a relatively smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish-white color, suggesting an older stellar population. There's a subtle transition into a fainter, more diffuse halo surrounding the core. This halo shows a bluer tint compared to the core, hinting at the presence of some younger stars or ongoing star formation, albeit at a low rate. The overall shape appears largely undisturbed, showing no significant signs of major mergers or tidal interactions. There might be subtle hints of faint, diffuse features in the outer regions, but these are not sharply defined. The galaxy appears to be relatively isolated in its environment.
