The galaxy presents as a single, relatively smooth, elliptical object. Its core exhibits a bright, concentrated luminosity, appearing yellow-orange. This suggests a considerable population of older stars within the nucleus. A less concentrated, yet still significant, halo extends outward from the core. The halo transitions to a greenish hue, possibly indicating the presence of younger stars or regions of ongoing star formation. The overall shape is generally round, although there is a slight elongation. No distinct spiral arms or bars are discernible. The galaxy appears relatively isolated, with no obvious signs of a major merger or significant tidal disturbance. There is a slight disturbance, however, possibly from a minor merger. The color profile indicates that this galaxy likely has moderate stellar mass and low star formation.
