The galaxy appears as an elliptical-type morphology, exhibiting a largely smooth light distribution with a centrally concentrated bulge. There is a slight elongation, though the overall shape is relatively round. The core is noticeably bright, suggesting a high concentration of stars and potentially an active galactic nucleus. The galaxy shows a color gradient, transitioning from a reddish-yellow center to a bluer outer halo. This color shift indicates a change in stellar populations, with older, redder stars dominating the core and younger, bluer stars present in the surrounding regions. There are indications of a minor disturbance or interaction, possibly a faint tidal feature or asymmetry in the outer regions, though the galaxy remains mostly undisturbed. Overall, this galaxy is a relatively massive system with moderate star formation activity.
