The galaxy presents as a somewhat elongated structure with a noticeable central bulge that appears yellowish-orange in color. This suggests an older stellar population concentrated towards the center. Extending outwards from the bulge is a disk component, although the disk is not clearly resolved into distinct spiral arms. The disk appears relatively smooth and patchy with some bluer regions, hinting at ongoing star formation within localized areas. The galaxy is moderately inclined with respect to our line of sight, offering a view of its three-dimensional structure. Overall, the galaxy seems to be relatively undisturbed with no obvious signs of major mergers or strong tidal interactions. There is, however, some irregularity in the disk, possibly indicating minor disturbances.
