The galaxy presents as a centrally concentrated, luminous object with an apparent smooth morphology. The central region exhibits a bright, concentrated core with a yellowish-white hue. This suggests the presence of an older stellar population. A fainter, bluish halo surrounds the core, extending outwards. This halo is more diffuse and less uniform in color, possibly indicating the presence of younger stars or ongoing star formation activity, albeit at a low level. No distinct spiral arm structures or dust lanes are visible. The overall shape appears approximately circular, with no obvious distortions or tidal features indicative of a recent major merger. However, some slight asymmetries in the outer halo may point to minor interactions or disturbances. The galaxy's size is moderately extended.
