This galaxy exhibits an overall smooth morphology. The central region shows a bright, concentrated bulge. Surrounding the bulge is a fainter, more diffuse disk-like component. There is little evidence of strong spiral arm structure or significant dust lanes. The galaxy is mostly symmetric, with a round shape, though it is slightly elongated. There may be a faint tidal feature or minor disturbance present, perhaps indicative of a past or ongoing interaction. The light from the galaxy is bluer in the outer regions, which could be a result of younger stellar populations.
