The galaxy presents as a moderately bright, elongated structure. It exhibits a smooth appearance with a central bulge that transitions into a flattened disk. The central region appears more concentrated and exhibits a yellowish hue, potentially indicating an older stellar population. The disk shows a bluer tint, which might indicate active star formation. The overall shape is strongly elliptical, resembling a cigar shape, with one end appearing slightly more diffuse. There is a suggestion of a faint, disturbed area near one of the outer edges of the galaxy, possibly indicating a minor interaction or internal disturbance. This does not look like an actively merging galaxy, but there may be evidence of past interaction.
