The galaxy presents an overall smooth morphology with a relatively symmetrical distribution of light. The central region exhibits a bright, concentrated core. The light appears bluer than the outer regions, indicative of a younger stellar population and possibly ongoing star formation. The outer regions of the galaxy appear fainter and redder, suggesting an older stellar population. There is some faint patchy structure, giving the impression of a weak disk component. The galaxy appears to be roughly rounded in shape, without any pronounced ellipticity or tidal features. There is no obvious sign of a major merger or strong gravitational interaction, although there are signs of a minor disturbance within the galaxy.
