The galaxy presents as a moderately bright, centrally concentrated system. It appears largely spheroidal in shape, exhibiting a smooth luminosity profile that decreases with distance from the central region. There is subtle evidence of a disk, though features are not prominent.

The galaxy displays a color gradient, with a central region that appears yellowish-white, transitioning to a bluer hue in the outer regions. The yellow-white hue of the central region suggests an older stellar population and possibly a dominant bulge component. The bluer color in the outskirts may indicate the presence of younger, hotter stars and ongoing star formation. Subtle disturbances or asymmetries could be present, suggesting the possibility of past minor interaction or merger events, though the overall structure is largely undisturbed. The overall morphology points to a galaxy in a state of ongoing, albeit perhaps relatively quiescent, evolution.
