The galaxy appears as a flattened, elliptical structure with a bright, concentrated central bulge that graduates into a diffuse disk. The color profile suggests an older stellar population in the bulge, indicated by the yellowish-orange hue, while the disk exhibits a bluer tint, hinting at the presence of younger, hotter stars and possibly some ongoing star formation.

The overall smoothness of the galaxy indicates a relatively relaxed state, with a notable absence of strong spiral arm structures or significant dust lanes. However, there is a hint of possible minor disturbance or interaction given the slight asymmetry in the outer disk region. The shape is predominantly in between round and cigar-shaped, indicating a moderate ellipticity.
