The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. There is an apparent lack of defined spiral arms or a prominent disk structure. The overall color appears somewhat yellowish-white, suggesting a population of older stars, although a slight bluer tint is present. The light appears to diffuse outwards in an almost perfect symmetrical gradient. There is little sign of significant ongoing star formation based on the light profile. There is a suggestion of minor disturbance, but nothing that would suggest this galaxy is currently undergoing a major merger event. The estimated size would appear to be between 1-2 kpc. 
