The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated with a bright, reddish core that gradually fades into the outer regions. There is a slight elongation, but it is mostly round in shape. The galaxy exhibits a color gradient, transitioning from a reddish hue in the center to a bluer tint in the outskirts. This color difference implies a variation in stellar populations, with the core likely dominated by older, redder stars, while the outer regions may contain younger, bluer stars or a different dust composition. No prominent spiral arms, bars, or significant dust lanes are visible. There are no obvious signs of major disturbances or ongoing mergers. The general appearance suggests a relatively evolved system with a likely quiescent star formation rate.
