This galaxy exhibits a generally smooth morphology. It appears to have a disk-like structure, but features are not prominent. There is a subtle central bulge, which seems somewhat extended and elongated. The object's color suggests a relatively older stellar population, and thus a low star-formation rate, although there may be regions of weak star formation. There is no evidence of any major mergers or strong tidal disturbances that could disrupt the galaxy's overall shape, though minor disturbances could be present. The light distribution indicates that the galaxy is moderately elliptical, rather than perfectly circular.
