The galaxy presents as a centrally concentrated object, with a notable degree of overall smoothness. The light distribution is dominated by a central bulge region which appears slightly elliptical. There is a hint of a disk structure, but it is faint and not well-defined, and the central bulge dominates the overall morphology. There is a subtle asymmetry in the galaxy's shape, perhaps indicative of a minor disturbance or interaction. The primary color of the galaxy is a pale yellow/white hue, suggesting a relatively older stellar population. There is some blue tint in the central region, which hints at an underlying amount of ongoing star formation. The object does not show signs of a major merger event, and the light profile is relatively regular. The apparent angular size is small, suggesting the galaxy is at a considerable distance.
