The galaxy presents a generally smooth, concentrated morphology with a slightly elongated, elliptical shape. It exhibits a bright central region which may indicate the presence of an active galactic nucleus or a concentrated stellar population. The galaxy's color gradient transitions from a bluer hue in the core to a subtly redder shade in the outer regions. There is some evidence of minor disturbances or faint features that could be indicative of tidal interactions or internal asymmetries, though these are not prominently defined. Overall, it appears to be a relatively isolated system with no strong signs of major recent mergers, and presents as a mildly disturbed elliptical or lenticular galaxy.
