The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light distribution appears centrally condensed, with a gradual decrease in surface brightness outward from the core. The color profile shows a redder core region, which may indicate an older stellar population or the presence of dust obscuration in the central regions. The outer regions of the galaxy exhibit a bluer hue, potentially indicating the presence of younger stars. There may be some minor disturbance in the galaxy's structure. The overall morphology appears undisturbed, with no major signs of on-going merging activity.
