The galaxy appears as a centrally concentrated object, exhibiting a smooth and featureless morphology. The light profile increases towards the center, suggesting a significant bulge component. The overall shape is moderately elliptical, neither perfectly spherical nor highly elongated. There is no readily apparent spiral arm structure or bar-like feature visible. The color is relatively uniform across the galaxy, trending towards a bluer hue in the outer regions and a yellower hue in the center. This color gradient may be indicative of an older stellar population dominating the central regions with younger stars in the outer regions. The galaxy seems relatively isolated. There is no obvious evidence of tidal disturbances or ongoing merger activity.
