The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. There is no readily apparent spiral arm structure or prominent disk component. The color profile exhibits a relatively homogenous distribution with a slight reddening towards the central regions, possibly indicative of an older stellar population dominating the core. The galaxy appears isolated, showing no strong signs of tidal interactions or major mergers, although there is a possibility of minor disturbances given some slight irregularities in its outer isophotes. The object has a generally rounded shape.
