The galaxy presents as a relatively smooth, elliptical structure, elongated in shape. It appears to lack distinct spiral arms or a well-defined central bulge. A bright, diffuse central region is apparent, suggestive of a concentration of older stars. There is a subtle color gradient, transitioning from a whiter core to bluer outer regions. The edges of the galaxy fade gradually into the background, indicating a smooth stellar distribution. There is a slight indication of internal dust lanes or faint features, but the overall impression is one of homogeneity. Some minor disturbances can be detected.
