The galaxy presents an elliptical morphology, exhibiting a smooth, generally featureless appearance. It has a concentrated central bulge that appears yellowish, indicating a population of older stars. The galaxy's light profile fades gradually outward from the core. There is no visible dust lane or spiral arm structure. Faint, diffuse extensions are present in what appears to be a minor disturbance or tidal interaction, hinting at a possible ongoing or past merger event. There may be a faint companion galaxy, as there are slightly brighter clumps of light at the very edge of the galaxy. These faint clumps could also be star forming regions.