The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, luminous core that gradually fades into a diffuse halo. The galaxy's color appears to be predominantly yellowish, suggesting a stellar population dominated by older, less massive stars. There is little evidence of significant dust lanes or spiral arm structures within the observed light. The overall shape approximates a rounded form, with minimal deviation towards an elongated or cigar-like appearance. There is no visually discernible evidence of ongoing major mergers or significant tidal disturbances influencing the galaxy's structure. A slight bluer tinge around the edges suggests there might be some recent star formation occurring at a very low rate in the outer regions.