The galaxy presents as a fairly symmetric elliptical or lenticular system, appearing largely smooth in texture with a concentrated central bulge. The light profile appears to decline steadily from the core outwards without any obvious breaks. The object exhibits a yellowish-white coloration, potentially indicative of an older stellar population. The lack of distinct spiral arm structures or intense blue star-forming regions supports this assessment. Overall, this galaxy seems to be a relatively evolved system with minimal ongoing star formation.
