This galaxy exhibits a generally elliptical morphology, displaying a smooth light distribution that transitions from a concentrated, reddish core to a bluer, more diffuse outer halo. There is an apparent lack of distinct spiral arm structures, suggestive of a relatively old stellar population distributed evenly throughout the galaxy. The central region presents a significantly redder hue than the outer regions, possibly indicating a higher concentration of older, redder stars or significant dust extinction. While the galaxy appears mostly undisturbed, there is a hint of asymmetry in the outer regions.
