The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central region, potentially indicative of a bulge. The light distribution appears mostly uniform, with no readily discernible spiral arms or significant dust lanes. The color profile suggests a population of older stars, with a yellowish hue dominating the central region and a slight bluer tinge towards the outer edges. There is no obvious evidence of ongoing major mergers or tidal disturbances, although faint, subtle irregularities in the outer halo cannot be entirely ruled out without deeper imaging. The object's apparent roundness points towards a low inclination angle relative to our line of sight. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
