The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that dominates its overall morphology. The luminosity profile appears to decrease steadily from the center outwards, with no distinct spiral arms or prominent star-forming regions visible. The galaxy exhibits a predominantly blue-green hue, suggestive of some ongoing, albeit likely subdued, star formation activity. There are no apparent signs of recent major mergers or significant tidal disturbances affecting the galaxy's shape. The overall appearance suggests a galaxy that is transitioning towards a more quiescent state, possibly an intermediate type between spiral and elliptical classifications. The isophotes appear generally regular and without sharp breaks, indicative of a relatively well-mixed stellar population.
