The galaxy appears as a roughly elliptical, smooth object with a concentrated central bulge. Its color gradient transitions from a yellowish core to a reddish-orange outer region. There is minimal visual evidence of spiral arm structure or prominent dust lanes, suggesting a relatively old stellar population with a low star formation rate. Possible minor distortions or irregularities in its outer regions may indicate a past or ongoing minor interaction with another galaxy, or an internal disturbance. The object displays an intermediate ellipticity, falling between perfectly round and elongated.
