The galaxy appears as a slightly elongated, centrally concentrated object. Its light profile suggests a relatively smooth distribution, with no readily apparent spiral arm structure. The galaxy has a somewhat round shape with light distributed in a relatively symmetric pattern. The color suggests a mix of stellar populations; redder hues are observed indicating the presence of older stars. The size of the galaxy is intermediate, neither extremely large nor particularly compact. There is no obvious evidence of a major merger or tidal disturbances. However, there is a hint of asymmetry, possibly indicating a minor interaction or internal dynamics affecting the overall structure.
