The galaxy presents an overall smooth appearance, lacking prominent spiral arms or a well-defined disk structure. The light is concentrated towards the center, indicating a significant bulge component. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, the galaxy gradually fades into a more diffuse, bluish envelope. The overall shape appears close to circular, showing a slight elongation. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although subtle irregularities in the outer regions might suggest minor past interactions.
