The galaxy presents as a centrally concentrated, elliptical-like morphology. The light profile appears relatively smooth, suggesting a lack of significant spiral arm structures or large-scale irregularities. The core region exhibits a bright, yellowish hue, which could indicate an older stellar population dominating the central bulge. A subtle color gradient is observed, transitioning to slightly bluer tones in the outer regions. This could suggest the presence of younger stars at larger radii, although the color shift is minimal. The overall shape is moderately elongated, deviating slightly from a perfectly circular form, with no obvious signs of ongoing major mergers or strong tidal interactions. The galaxy shows a considerable mass and its likely undergoing moderate star formation, possibly in the last stages of its evolution.
