The galaxy presents as a predominantly smooth, elliptical object with a concentrated central bulge. The core exhibits a yellowish hue, suggestive of an older stellar population. A diffuse, fainter halo surrounds the central region, gradually fading into the background sky. The galaxy appears moderately elongated, but generally rounded in shape. There is no strong evidence of spiral arm structure or significant dust lanes. Minor disturbances and features were not readily apparent. The overall color profile indicates a relatively low star formation rate. The galaxy is estimated to be a supermassive galaxy.
