The galaxy presents as a relatively smooth, elliptical-like object. Its central region exhibits a higher luminosity, appearing bright and concentrated. There is a subtle color gradient between the central bulge and the outer regions. The core appears yellowish, possibly indicating an older stellar population. Moving outward, the galaxy gradually fades, with a slight bluish tinge in its surrounding halo. There is a subtle disk shape, and the galaxy appears to be more oblong than perfectly circular. The edges of the galaxy lack sharp definition, suggesting a diffuse stellar distribution in the outer regions. There is no readily apparent evidence of recent or ongoing major mergers or tidal disturbances.
