The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The color appears to be primarily blue-white, potentially indicating a substantial population of younger, hotter stars. A faint disk component may be present, as suggested by the slightly elongated shape. There is a slight indication of minor disturbances in the outer regions, possibly suggesting ongoing or past interaction with another galaxy, but that seems unlikely. Overall, the galaxy appears to be relatively smooth in texture, with the bulk of its stellar population concentrated towards the center.
