The galaxy presents as a roughly circular object with a smooth, centrally concentrated light distribution. The central region exhibits a bright, almost stellar-like core, surrounded by a more diffuse halo of light. There is evidence of a slight color gradient, with the central core appearing bluer than the outer regions. There are suggestions of minor disturbances in the smooth, outer parts of the galaxy, but it's difficult to determine whether they are tidal tails, stellar streams, or artifacts. Overall, the galaxy appears to be relatively isolated, showing no strong signs of a major ongoing merger, and it seems more elliptical than spiral.
