The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, with only slight deviations from perfect roundness. The central region displays a pronounced brightness, suggesting a substantial concentration of stars and potentially a supermassive black hole actively accreting material. A color gradient is observed, transitioning from a yellowish hue in the core to a slightly bluer tint in the outer regions. This suggests a shift from older stellar populations in the center towards younger, hotter stars in the galaxy's outskirts, possibly indicative of ongoing or recent star formation. There is no obvious evidence of spiral arms or a prominent disk structure. No signs of major mergers or tidal disruptions are readily apparent.
