The galaxy presents as a lenticular or possibly an edge-on spiral galaxy, viewed at a significant distance. It appears elongated, with a length-to-width ratio suggesting a flattened structure. The central bulge is not very prominent but is noticeable with a slightly brighter, more concentrated light profile. There is a general smoothness to the overall structure, with minimal evidence of spiral arm structure or prominent dust lanes. The color gradient indicates a likely older stellar population and low rate of star formation. The lack of clumpy or irregular features suggests no major mergers or significant tidal disturbances are currently affecting the galaxy. There may be some minor disturbances but none are apparent. The galaxy is dominated by intermediate age or older stars, and little gas for further star formation.
