The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular, with a high degree of radial symmetry. A bright, concentrated central bulge dominates the overall light distribution. There is no readily apparent spiral arm structure or dust lane. Some faint and diffuse features surround the central region, perhaps indicative of a faint halo or tidal debris, or minor interactions. The galaxy exhibits a color gradient, with a bluer hue towards the outer regions and a redder color in the core. This color change likely signifies variations in the stellar population, perhaps with the presence of older, redder stars concentrated in the nucleus.
