The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with a bright, concentrated central bulge.  There appears to be a subtle disk component. The galaxy's color profile suggests a population of older stars, indicated by the reddish-yellow hue. Faint spiral structure is observable within the disk. The lack of sharp features or prominent dust lanes implies a relatively quiescent state of star formation. The overall symmetry indicates it is not undergoing a major merger, although there are some small asymmetric disturbances suggesting minor tidal interactions may be occurring. The galaxy is estimated to be of significant mass. 
