The galaxy presents a generally smooth morphology, with no immediately obvious spiral arm structure or significant dust lanes. Its shape is largely elliptical, appearing more intermediate in roundness rather than perfectly circular or highly elongated. The light distribution is concentrated toward the center, with a gradual decrease in brightness outwards. There is no strong evidence of ongoing major mergers or significant tidal disturbances; however, subtle irregularities in the outer regions may suggest minor interactions or past disturbances. Overall, the galaxy appears as a relatively undisturbed system, exhibiting a redder color indicative of an older stellar population and lower current star formation activity.
