This galaxy presents as an elliptical type, exhibiting a generally smooth, centrally concentrated luminosity profile. The core region shows a yellowish hue, suggestive of an older stellar population dominated by redder stars. The galaxy appears to be relatively spheroidal, deviating only slightly from a perfectly circular shape. There is no evidence of distinct spiral arms or a prominent disk structure. Faint bluer regions are observed in the outer areas of the galaxy, which may indicate some regions of ongoing low-level star formation. No obvious signs of tidal disturbances, mergers, or interacting companions are apparent. The overall morphology indicates a galaxy that has likely undergone significant dynamical relaxation, with minimal recent interaction history.
