The galaxy appears to be a relatively smooth, elliptical galaxy exhibiting a slightly elongated shape. It possesses a bright, concentrated central bulge that gradually fades into a more diffuse outer halo. The color gradient transitions from a yellowish-white core, potentially indicative of an older stellar population, to a redder hue in the outer regions, which suggests a possible presence of dust absorption or an aging stellar population away from the center. No distinct spiral arms or prominent dust lanes are discernible within the galaxy's structure. There is no evidence of major morphological disturbances or ongoing merging activity. The galaxy exhibits no characteristics of star formation, based on the smooth features and older populations.
