The galaxy presents as a somewhat elliptical structure. The central region exhibits a higher surface brightness, appearing as a concentrated, bright core. Moving outwards, the luminosity gradually decreases, fading into a more diffuse halo or disk. A slight elongation is visible, with the galaxy appearing more cigar-shaped than perfectly circular. There is no obvious spiral arm structure or any clear signs of major disturbances, such as tidal tails or asymmetries, though there may be some indication of minor disturbances. The overall color profile suggests a relatively evolved stellar population. Based on these observations, this galaxy likely represents an early-type galaxy, specifically an elliptical, with a modest estimated size.
