The galaxy presents as a moderately bright, elliptical-shaped structure with a smooth appearance. The central region exhibits a yellowish hue, suggesting an older stellar population and diminished recent star formation activity. The outer regions of the galaxy appear fainter and bluer in comparison, possibly indicating the presence of younger, bluer stars, or simply a lower density of stars overall. There is a slight elongation observed, with the major axis oriented roughly horizontally in the image. The galaxy lacks any distinct spiral arm structures or prominent dust lanes. No major mergers or significant tidal disturbances are immediately apparent, although there are potentially subtle irregularities in the outer regions. Based on the galaxy's color and smooth morphology, it is likely a relatively massive system composed of primarily older stars, with star formation occurring at a lower rate.
