The galaxy presents an elliptical morphology, appearing as a flattened spheroid. The central region exhibits a high surface brightness, displaying a yellow-white coloration, suggestive of an older stellar population dominating the core. The isophotes show significant flattening, with an ellipticity measurement that indicates a deviation from a perfect circle. A faint, diffuse halo surrounds the central bulge, gradually fading into the background sky. There appears to be a slight asymmetry or disturbance on one side, potentially indicative of a minor interaction or merger event. The overall color gradient shows a shift towards bluer hues in the outer regions, implying the presence of younger, star-forming regions in the disk. The galaxy demonstrates a relatively smooth appearance, lacking prominent spiral arm structures.