The galaxy presents as a centrally concentrated elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. The core is bright and compact, suggesting a high stellar density and possibly an active galactic nucleus, though no clear jet is visible. The galaxy's light profile appears spheroidal, gradually decreasing in intensity from the center outwards. There is a slight color gradient observed, where the inner region tends toward the yellow and the outer region appears to be slightly more blue. This may indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars found in the outer regions. There are no distinct spiral arms, bars, or strong dust lanes visible, further supporting its classification as an early-type galaxy. The overall symmetry and smooth texture suggest that it is not currently undergoing any major merging events, although a slight irregular region may be indicative of a minor tidal disturbance. Its half-light radius appears small, indicating it may be relatively compact.
