The galaxy presents as a relatively smooth, centrally concentrated object. It appears approximately round, with a slight elongation. The color profile suggests a redder central region, possibly indicative of an older stellar population. The lack of distinct spiral arms or prominent dust lanes suggests a classification toward the elliptical end of the Hubble sequence. There is no obvious evidence of strong tidal interactions or major mergers, although some subtle disturbances cannot be ruled out. The galaxy appears relatively isolated in the field of view. Overall, the galaxy's morphology is consistent with a passively evolving system.
