The galaxy presents as a relatively smooth, elongated structure, exhibiting a concentrated central bulge. The morphology suggests a likely classification as an elliptical galaxy, though some disk-like features cannot be entirely ruled out due to the resolution. The light distribution appears to be centrally concentrated with a gradual decrease in brightness towards the outer edges. The colors are somewhat uniform across the galaxy with a hint of redder hues in the central region, transitioning to slightly bluer tones in the outskirts, indicative of a stellar population with potentially ongoing, but moderate, star formation. There is no distinct evidence of spiral arms or significant dust lanes. Minor irregularities along the edges hint at possible gravitational interaction. The overall structure suggests a system undergoing relatively quiescent evolution.
