The galaxy presents as a somewhat elongated, centrally concentrated object. Its color gradient transitions from a yellowish core to a slightly bluer periphery. The central region exhibits a smooth, featureless appearance indicative of an older stellar population. The outer regions show hints of a fainter disk-like structure. A slight distortion or irregularity is present on one side suggesting potential interaction or minor disturbance, but no obvious signs of ongoing major mergers. Overall, the galaxy appears as an intermediate-mass system with a likely significant spheroidal component, moderate star formation activity in its outer regions, and a possible history of gravitational interaction.
