The galaxy presents as an elliptical-like structure with a bright, concentrated central bulge. The galaxy exhibits a smooth texture, lacking prominent spiral arms or distinct features indicative of active star formation in the outer regions. The overall light distribution suggests that the galaxy is dominated by an older stellar population, with the central bulge appearing more luminous than the surrounding halo. The ellipticity is visible, indicating a deviation from a perfect spherical shape. The lack of observable dust lanes or significant color variations further supports the classification of this galaxy as an early-type system. A faint, diffuse halo surrounds the central region, gradually fading into the background.
