The galaxy presents a largely smooth, elliptical morphology with a slight elongation visible in its overall shape. It exhibits a fairly concentrated light profile, with a gradual decrease in intensity from the center outwards. There is no strong evidence of prominent spiral arms or a well-defined disk structure. A subtle colour gradient is observable, with the central region appearing somewhat redder, suggesting an older stellar population dominating the core, while the outer regions display a slightly bluer tint, potentially indicating the presence of younger stars or ongoing star formation, albeit at a low rate. There are no obvious signs of major mergers or tidal disturbances affecting the galaxy's structure. Small irregularities are seen, though are minimal. Overall, the galaxy appears to be an evolved system with a predominantly old stellar population and a quiescent star formation history.
