The galaxy exhibits a generally smooth morphology, appearing elliptical in shape. Its color profile is predominantly yellowish-white, suggestive of an older stellar population. There is a slight central concentration of light intensity, indicating a possible nucleus or bulge. No distinct spiral arms or significant dust lanes are discernible within the galaxy's structure. There is some evidence of faint, diffuse outer regions, indicating a gradual decline in stellar density from the core to the periphery. The galaxy appears relatively undisturbed, with no clear signs of ongoing major merger activity or significant tidal distortions.
