The galaxy presents an overall elliptical morphology, appearing somewhat flattened. The central region exhibits a concentrated luminosity, gradually decreasing towards the outer edges. The galaxy appears largely featureless, without any readily apparent spiral arms or distinct structures. Color gradients are subtle, with a slightly bluer hue in the outer regions compared to the yellowish-white central bulge. The light distribution suggests a relatively smooth stellar population. There are no obvious signs of ongoing major mergers or significant tidal disturbances within the system.