The galaxy presents as a single, relatively smooth light distribution, with no apparent spiral arms or prominent disk structure. The central region exhibits a strong concentration of light, suggesting a prominent bulge. The overall color appears to be trending toward redder wavelengths, with the central bulge slightly more yellow-orange than the outer regions. There are no obvious signs of significant tidal disturbances or ongoing major mergers, as the light distribution is largely undisturbed and symmetric. Faint, diffuse blue light is visible in the outer areas, suggesting a low level of star forming regions or younger stars distributed in the surrounding regions. The elliptical shape appears close to circular, indicating a near face-on orientation.
