The galaxy presents as a somewhat elliptical structure, though closer to being in between round and cigar-shaped. A central bulge is visible, appearing bright and relatively smooth, suggesting an older stellar population. Fainter, bluer regions extend outwards from the central bulge, indicating the presence of some ongoing star formation within what appears to be a disk or spiral arm structure. The galaxy does not appear to be undergoing any major mergers, although a minor disturbance is apparent in the outer regions, possibly from a past interaction. Overall, the galaxy appears to be a relatively massive system exhibiting a mix of old and young stellar populations, with modest star formation activity.
