The galaxy appears to be an elliptical type, exhibiting a generally smooth and centrally concentrated morphology. The light distribution suggests a spheroidal shape, being mostly round. There may be a very faint, diffuse halo surrounding the brighter central region, although the signal is weak.

There is a noticeable color gradient, with the core displaying a yellowish-white hue, possibly indicating a population of older stars. The outer regions appear slightly bluer, implying the presence of some younger stellar populations. However, the blue component is subdued, which suggests that active star formation is either low or absent. 

There is no discernible spiral structure or prominent dust lanes visible in this image. There is no major ongoing merger apparent in the image, though subtle irregularities could be indicative of a past interaction. 
