The galaxy appears as a fairly smooth, centrally concentrated object. Its morphology is generally rounded, exhibiting only a slight deviation from perfect circularity. While a significant portion of the light is concentrated in the center, there is evidence of a diffuse, extended halo surrounding the core. The color profile suggests a moderately blue spectral energy distribution in the halo, with the central regions exhibiting an even more blue-shifted color profile. Faint, asymmetric features are visible in the galaxy's light distribution, suggestive of minor disturbances.
