The galaxy presents a somewhat elliptical morphology, appearing more rounded than elongated. The central region exhibits a brighter concentration of light, suggesting a prominent galactic nucleus. A diffuse halo surrounds this central area, fading into the background. Some irregularities in the outer regions indicate the presence of either tidal disturbances or ongoing star formation. Overall, the light distribution seems relatively smooth, indicating it is likely an early-type galaxy with no obvious spiral arms. The galaxy appears to be relatively isolated.
