The galaxy presents as a relatively compact, elliptical-like structure with a smooth, centrally concentrated light distribution. There appears to be some subtle color variation within the galaxy, with a slightly redder core compared to the outer regions. There are no readily apparent spiral arms or prominent dust lanes, suggesting a lack of significant recent star formation. The overall morphology indicates that this is likely an evolved galaxy, possibly a massive elliptical with an older stellar population. There are no obvious signs of tidal features or ongoing major mergers, indicating the galaxy is relatively isolated.
