The galaxy presents as a generally smooth and centrally concentrated object. Its morphology is broadly elliptical, with a slight deviation towards a prolate, cigar-like shape. The light distribution is dominated by a bright central bulge, with a gradual decline in intensity towards the outer regions. There is little evidence of spiral arms or prominent disk features. A subtle color gradient is observed, transitioning from a yellowish-white hue in the core to a slightly redder tint in the outer regions. This suggests a stellar population gradient, with potentially older, redder stars dominating the outskirts. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of ongoing major mergers or significant tidal interactions. Some minor asymmetries are visible within the galactic disc but are mostly subtle.
