The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is elliptical or spheroidal, displaying a high degree of roundness. There is a gradual decline in surface brightness from the core outwards, without any distinct spiral arm structures or prominent features indicative of a disk component. The central region exhibits a yellowish hue, suggestive of an older stellar population. Fainter bluish light can be observed extending away from the center, indicative of some younger, bluer stars and possibly star formation. No signs of significant tidal disturbances or ongoing mergers are immediately apparent.
