The object presents as a relatively smooth, centrally concentrated galaxy with a discernible, yet subtle, disk-like structure. Its overall shape is generally round, displaying only a slight deviation toward an elliptical morphology. The color profile indicates a potential redder core region, shifting to bluer hues in the outer disk, suggesting the presence of younger stellar populations away from the galactic center. While generally smooth, there's some indication of minor structural disturbance or irregularity in the form of a slight asymmetry or a faint tidal feature, suggesting a possible interaction or recent merger event. A faint, extended halo surrounds the main galactic structure. The overall impression is of a galaxy transitioning perhaps from an elliptical to a more disk-dominated system, or recovering from a minor gravitational interaction.
