The galaxy presents a generally smooth, elliptical morphology. The light profile is concentrated towards the center, indicating a significant bulge component. Color gradients are apparent, transitioning from a yellowish hue in the core to a redder color in the outer regions. There are no prominent spiral arms or distinct dust lanes visible, which supports a classification towards the elliptical side. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers. Faint, diffuse halo extends from the central region. The overall appearance suggests a evolved system with a relatively old stellar population.
