The galaxy presents as a somewhat elongated structure with a smooth, featureless appearance. The central region exhibits a higher surface brightness, suggesting a concentration of older stellar populations or a bulge component. The overall color is slightly red, implying that it is an older galaxy, likely an elliptical, with a low rate of star formation. There is a very slight hint of a disc-like structure, but this is minimal. No evidence of spiral arms, star-forming regions, or significant dust lanes are visible. The galaxy appears to be relatively isolated, showing no clear signs of interaction or merging with nearby galaxies. The edges are well defined, and the lack of tidal features further support the assessment that it is a settled, mature system.
