The galaxy appears to be a relatively smooth and rounded structure, lacking any obvious spiral arms or a prominent disk. It presents a concentrated central bulge that transitions smoothly outward. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population within the bulge. The outer regions of the galaxy show a faint bluish tint, suggestive of some ongoing star formation, though at a low rate. There is no clear evidence of tidal features, major mergers, or significant disturbances in its overall morphology. The galaxy exhibits a compact appearance with no distinct or resolvable substructures.
