The galaxy presents as a centrally concentrated object with a generally smooth morphology, exhibiting a flattened, elliptical appearance. The primary color of the central region is a yellowish-white, suggesting an older stellar population. Fainter, bluer tendrils of light extend from the central bulge into the surrounding halo, potentially indicating regions of more recent, though subdued, star formation. There is a slight asymmetry to the outer halo, but no clear evidence of ongoing major merger activity or strong tidal disturbances. The galaxy appears relatively isolated, showing no prominent companion galaxies within its immediate vicinity. Its overall structure is consistent with an early-type spiral or lenticular galaxy, where the star formation rate is relatively low.