The galaxy presents as an elliptical morphology with a dominant, smooth structure. The central region exhibits a bright, concentrated luminosity that gradually decreases towards the outer edges. Color gradients are subtle, with the core appearing slightly more yellow, transitioning to a faint, bluer hue in the outskirts. There is little evidence of significant star formation, spiral arms, or a prominent disk-like structure. It is primarily a spheroid, and displays no indication of ongoing major merging activity, though a subtle irregularity suggests the possibility of a minor disturbance, potentially from a past interaction or minor accretion event. The overall appearance is consistent with a relatively quiescent galaxy, possibly a more evolved system with a largely older stellar population. 
