The galaxy presents an apparent angular size of approximately 2.7 arcseconds, estimated by doubling the Petrosian half-light radius. The morphology of the galaxy appears predominantly smooth, suggesting a relatively high degree of sphericity. The central region exhibits a slightly more concentrated luminosity profile compared to its outer regions. There is an indication of minor disturbances in the overall structure and a slight elongation of the galaxy, though the galaxy appears round in general. The galaxy exhibits a color gradient from the center outward, with the central bulge appearing more yellow/orange. This color suggests the presence of an older stellar population.
