The galaxy presents as a relatively smooth, elliptical or lenticular system with a concentrated central bulge. The light distribution appears consistent with an evolved stellar population, exhibiting a general lack of distinct spiral arm structures. The galaxy's overall shape is nearly circular, with a slight elongation along its major axis. There is a gradual decrease in surface brightness from the core outwards, indicating a centrally concentrated mass distribution. No significant dust lanes or prominent star-forming regions are clearly discernible within the galaxy's structure. The galaxy has a redshift indicating a substantial distance.
