The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. There is little evidence of spiral arms or a distinct disk structure. The object appears fairly round. The color gradient suggests a population dominated by older stars, potentially with a redder, more evolved stellar population. No significant dust lanes or regions of active star formation are immediately apparent. The galaxy exhibits a relatively undisturbed structure, with no indications of ongoing mergers or major tidal interactions.
