This galaxy appears to be a relatively smooth, disk-dominated system. It is elliptical in shape, with an approximate axis ratio of roughly 2:1. The light distribution is centrally concentrated, with a bright nucleus that fades gradually into the outer regions. There is evidence of a slight color gradient, the central region appears yellowish suggesting an older stellar population. Fainter bluer regions are visible within the disk, potentially indicating the presence of ongoing, albeit low-level, star formation. There is no clear indication of spiral arms or a bar-like structure. No obvious signs of tidal disturbances, major mergers, or significant interactions with nearby galaxies are detected in this image.
