The galaxy presents a largely smooth, elliptical morphology, suggesting a classification towards the earlier end of the Hubble sequence. The light distribution is concentrated towards the center, with a distinct bulge component. The core is bright and has a yellowish hue, suggestive of an older stellar population. There is a lack of discernible spiral arm structure or significant dust lanes within the galaxy. The outer regions exhibit a gradual decrease in luminosity with increasing radius. The overall appearance indicates a relatively quiescent galaxy, without significant ongoing star formation. There is no obvious evidence of any tidal disturbances or mergers affecting its morphology.