The galaxy presents as a generally smooth and elongated structure, exhibiting a pronounced disk-like morphology with an elliptical shape. There is a slight indication of a central bulge, though it is not particularly dominant. The galaxy's light profile seems to be relatively smooth, with a gradual fading towards the outer edges, which may indicate a well mixed population of stars. I do not see a prominent dust lane or intense spiral arm structure. In general, the galaxy appears to be fairly settled. The color distribution shows a slight gradient, with the central regions exhibiting a slightly yellowish to white hue, potentially indicating an older stellar population, with hints of bluer tones extending outwards in the disk, suggesting more recent star formation activity. The galaxy shows no obvious signs of a major ongoing merger event, although there may be some minor distortions.
