The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a high degree of central concentration, with luminosity decreasing gradually from the core. The color is generally yellow-red, suggestive of an older stellar population and a lower rate of current star formation. There is no apparent spiral arm structure or significant dust lane features visible. The overall shape appears nearly circular, indicating a relatively low degree of flattening. There is no evidence of ongoing major merger activity or significant tidal disturbances, with some possibilities of a minor disturbance. 
