The galaxy presents an overall elliptical morphology, with a smooth, diffuse appearance. The light distribution suggests a centrally concentrated luminosity profile, becoming fainter towards the outer regions. Color gradients are subtle, with a slightly yellower hue dominating the central region, potentially indicating an older stellar population. There are no distinct spiral arms or significant dust lanes visible. There appears to be a very slight flattening of the galaxy which gives it the shape of a plump football. No signs of any ongoing major merging events are observed, though there is some evidence of a small disturbance.