The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a centrally-peaked luminosity profile, with the brightest region residing within the core. The morphology indicates it is largely undisturbed, showing no signs of significant tidal features, close companions, or ongoing major mergers. There is a slight hint of a disk structure, though the dominant feature remains the smooth spheroidal component. Color gradients appear to be minimal with a somewhat homogeneous color profile indicating an old stellar population with low star formation. Overall the galaxy is well-defined and does not present any morphological irregularities.
