The galaxy presents as a centrally concentrated, relatively smooth object. Its morphology appears elliptical, with a gradual decrease in luminosity from the core outward. There is a slight elongation, but it is close to round. The color gradient across the galaxy is subtle, with a bluer central region suggestive of younger stellar populations. The galaxy is largely undisturbed, without apparent major tidal features or signs of ongoing or recent merger activity. There may be evidence of minor disturbances, however, such as a slightly irregular shape. The inferred size is consistent with dwarf galaxies.
