The galaxy appears as a somewhat elongated, cigar-shaped object. It exhibits a relatively smooth morphology, with a bright, concentrated central region suggestive of a bulge. The outer regions show hints of a fainter, disk-like structure, although distinct spiral arms are not readily apparent in this image. The color gradient suggests some variation in stellar populations. The central region is generally more yellow-white, possibly indicating older stellar populations. The disk appears bluer, potentially indicating ongoing or recent star formation. There might be some dust lanes or patchy star formation regions. The galaxy appears relatively isolated, without any signs of major mergers or strong tidal disturbances. There is a minor disturbance on one side of the galaxy.
