The galaxy presents as an elliptical morphology. It appears largely smooth in texture, with a concentrated central bulge. The light distribution suggests a relatively old stellar population, displaying a distinct reddish-orange hue. There is no apparent spiral arm structure or significant dust lane obscuration visible at this resolution. The overall shape is moderately elongated, showing a cigar shape. There is no indication of major disturbances or ongoing mergers, although subtle asymmetries might hint at minor gravitational interactions. 
