The galaxy appears to be a relatively smooth, rounded system. It exhibits a concentrated central bulge that graduates outward into a fainter disk. The light from the central bulge is yellowish, suggestive of an older stellar population. The disk light is slightly bluer than the central region, which may indicate more recent or ongoing star formation. The galaxy's shape is generally round with minimal visual disturbances or asymmetries, such as tidal tails. It also displays no obvious spiral arm structure or bar feature.
