The galaxy presents as a generally smooth object with a concentrated central bulge. There is little apparent structure or indication of spiral arms; no clear disk is visible. The morphology is roughly elliptical or lenticular. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a redder halo, suggesting an older stellar population. The object appears relatively isolated, showing no signs of ongoing major mergers or significant tidal interactions. The overall roundness suggests a relaxed dynamical state, with minor, if any, disturbances evident.
