The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. Color gradients are subtle, with the core exhibiting a yellow-white hue, transitioning to a redder and more diffuse outer halo. There's no clear evidence of spiral arms or a distinct disk. The light distribution is fairly even with no significant dust lanes or knots of star formation visible in the image. The overall morphology suggests an older stellar population, consistent with a lack of ongoing major star formation events. There is no visually-detectable interaction with any neighboring galaxies, nor evidence of a recent major merger. The galaxy appears relatively undisturbed.
