The galaxy appears as a centrally concentrated, elliptical-like object with a smooth, diffuse light profile. The core region exhibits a bright, yellowish-orange hue, suggesting a significant population of older stars. The galaxy's color becomes slightly bluer towards the outer regions, which may indicate a small population of younger stars or ongoing low levels of star formation. There is little evidence of spiral arms or a well-defined disk structure. The overall morphology appears undisturbed, showing no signs of major mergers or significant tidal interactions. The axial ratio indicates that it may be closer to spheroidal, and without prominent features. There is a slight inclination relative to our line of sight, as it is not perfectly circular.
