The galaxy appears as a single, relatively smooth and rounded object. It presents a concentrated central region that emanates light with a yellow tint, suggesting an older stellar population. The light profile gently fades outwards from the center, diminishing in intensity. No spiral arm structures, bars, or dust lanes are readily apparent from the image. No significant tidal features or signs of recent major mergers can be discerned. There is some indication of minor irregularities in the extended halo region.
