The galaxy presents as a slightly elongated spheroid. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or active galactic nucleus. Moving outwards from the core, the luminosity gradually decreases. The color appears to shift from a warmer yellowish hue near the center to a cooler, redder tone in the outer regions. There is some indication of a disk-like structure, although it appears relatively featureless. The overall morphology leans towards a smooth distribution of light, with no immediately obvious signs of spiral arms, strong dust lanes, or major disturbances indicative of recent mergers, though subtle irregularities may be present upon closer inspection. The galaxy's axial ratio suggests a possible classification as an elliptical galaxy viewed at an oblique angle, or potentially a lenticular galaxy.
