The galaxy presents an overall elliptical morphology, displaying a relatively smooth and centrally concentrated light distribution. The core exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, bluer light surrounds the core region, suggestive of ongoing star formation. The outer regions of the galaxy show a gradual decrease in luminosity. There are some subtle features or disturbances that may indicate a minor interaction or possible merger remnant. The galaxy does not appear to display any prominent spiral arm structure. 
