The galaxy presents as a diffuse, relatively smooth structure. It appears largely elliptical in shape, with a high degree of central concentration. There is little evidence of spiral arms or a prominent disk component. The color is generally redder, with a slight central yellowing. No major disturbances or tidal features are readily apparent, although there may be minor asymmetries that could indicate recent or ongoing interactions. The light distribution suggests a well-mixed population of older stars. Star formation appears moderate in the region. The estimated size is approximately 6 kpc in radius. There is a lack of any distinct dust lanes or regions of intense star formation. The galaxy presents a generally undisturbed and evolved morphology.
