The galaxy presents a generally elliptical morphology with a smooth, diffuse light distribution. There is a bright central bulge or core which is likely the location of a supermassive black hole. The galaxy exhibits a slight flattening of the ellipse. Faint outer regions extend beyond the central body of the galaxy, with a gradual decline in surface brightness. No distinct spiral arms or prominent dust lanes are observed. The galaxy exhibits a color gradient, appearing slightly redder in the central regions and becoming marginally bluer towards the outer edges. The apparent angular size suggests that it is a relatively nearby galaxy. The light profile appears smooth and well-fitted by a Sersic profile. There is no sign of major mergers or tidal disturbances.
