The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that fades gradually into the outer regions of the galaxy, displaying a minimal presence of defined spiral arms or prominent features. The overall color profile suggests a population of older stars, indicated by its reddish-yellow hue, consistent with low star formation activity. The round morphology implies a relaxed system, potentially having undergone previous mergers or interactions. No significant tidal tails or morphological distortions are apparent, suggesting it's a relatively isolated system without ongoing major interactions.
