The galaxy presents a generally smooth, elliptical morphology, though there is a hint of a disk-like structure. Its shape is observed to be moderately rounded, not strongly elliptical or cigar-shaped. Color gradients indicate the presence of a dominant population of older stars, visible as a yellow-orange hue in the central region, and bluer color is detected in the outer regions. There is no obvious dust lane or patchy dust distribution. There are no signs of strong tidal features, mergers, or major disturbances in its morphology, suggesting it is a relatively settled system. The light distribution suggests the presence of a bulge and a possible disk component.
