The galaxy appears as a relatively compact object with a roughly elliptical morphology. Its light distribution seems smooth, suggesting a lack of significant spiral arm structure or prominent star-forming regions in this particular image. There is a color gradient, with a slightly bluer hue concentrated in the central region. This may indicate the presence of a younger stellar population compared to the outer regions, which appear redder, possibly due to older, cooler stars or dust obscuration. There are hints of asymmetry but this could simply be due to the limited image resolution. No tidal tails or other signs of recent major merger activity are immediately apparent.
