The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a high degree of central bulge dominance observed, with the light intensity decreasing gradually from the core to the outer regions. No prominent spiral arm structures or distinct dust lanes are visible. The galaxy appears to be relatively undisturbed with no obvious signs of tidal interactions or ongoing mergers. Its color profile is red, suggesting an older stellar population and a relatively low rate of recent star formation. The overall roundness is notable. A faint, diffuse halo may be present.
