The galaxy presents as a relatively smooth, featureless object. It is elliptical in shape, with an axis ratio that suggests it is not highly elongated, but rather somewhere in between circular and cigar-shaped. A bright central bulge is visible, with a slightly reddish hue, indicating a concentration of older stars. Moving outward from the core, the galaxy exhibits a diffuse disk component with a bluer color, suggesting the presence of younger, hotter stars.

The overall structure appears relatively undisturbed, though there may be some minor asymmetry or faint irregularities in the outer regions, potentially hinting at past or ongoing interactions. There is no evidence of a major merger or significant tidal disturbances. The observed color gradients suggest ongoing, but not extremely intense, star formation within the disk.
