The galaxy presents as an elliptical morphology, exhibiting a smooth and featureless structure. The light profile is centrally concentrated, with a bright core that gradually fades into a diffuse halo. The color appears relatively uniform across the galaxy, with a subtle shift towards redder hues in the central regions, suggesting an older stellar population. There is no obvious evidence of spiral arms, dust lanes, or active star formation regions visible in this image. The overall shape is slightly elongated, deviating marginally from a perfect circle, but it does not suggest any ongoing major mergers or tidal disturbances. There may be some minor disturbances from a small gravitational interaction.