The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There appears to be little to no discernible disk component. The light distribution suggests a centrally dominant luminosity profile, fading gradually toward the outer edges. The core region exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions show a subtle shift towards redder colors, also consistent with an older population and minimal ongoing star formation. No clear spiral arms or dust lanes are visible. The overall morphology points towards a galaxy with a quiescent star formation history and a well-established structure, indicative of an evolved system. There are no apparent signs of major mergers or tidal disturbances, though some minor asymmetry cannot be entirely ruled out.
