The galaxy presents as a relatively smooth, elliptical-type galaxy, with a concentrated central bulge that appears very bright. The overall shape is more lenticular than perfectly spherical, exhibiting a slight elongation. No distinct spiral arms or features indicative of active star formation are visually apparent. The galaxy lacks pronounced dust lanes or asymmetries, suggesting it is not undergoing a major merger or significant tidal disruption. The color appears slightly reddish, potentially indicative of an older stellar population. The overall impression is that of a mature galaxy, potentially undergoing quenching or with low ongoing star formation.
