The galaxy presents as largely smooth in appearance, with a concentrated central bulge that dominates its overall luminosity. A faint, diffuse disk is discernable, extending outwards from the central region. The galaxy appears nearly circular, indicating a face-on orientation relative to our line of sight. There are subtle hints of possible minor disturbances in the outer regions of the disk, potentially indicative of past or ongoing interactions. The galaxy exhibits a yellowish-white hue overall, suggesting a population of older stars, although some bluer regions may be present, indicative of more recent star formation activity.
