The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that transitions smoothly into the outer regions. The galaxy's shape is somewhat elongated, appearing more "in between" round and cigar-shaped. No prominent spiral arms or bar structures are discernible. There is a subtle color gradient, shifting from a yellowish hue in the core to a bluer tint in the outer edges. This implies a variation in stellar populations, with older, redder stars likely dominating the central regions and younger, bluer stars residing in the outskirts. There's no clear evidence of ongoing major merger activity, although slight disturbances or minor interactions can't be ruled out based on the available imagery. The general appearance suggests a galaxy that has largely settled into a stable, post-starburst state, with relatively low levels of current star formation.
