The galaxy presents as a relatively bright, disk-like structure, observed at an inclination. A central bulge is visible with a yellow hue. The disk itself appears to have faint spiral arm structures with some blue light, though the resolution limits detailed observation. The overall color suggests a mix of stellar populations, with a significant presence of older stars. There is no obvious evidence of ongoing major mergers or tidal disruptions, although some minor disturbances may be present. The galaxy appears moderately massive, with a relatively low star-formation rate, suggesting a transition or quiescent state. It is mostly classified as a smooth object.
