The galaxy presents as a single, relatively smooth and concentrated luminous body. The central region exhibits a bright, high-intensity core that gradually diminishes in luminosity towards the outer edges. The morphology appears largely elliptical, with an approximate effective radius of 7 kpc. The color profile is predominantly yellow to orange, suggesting a population of older stars with lower rates of recent star formation. There are no obvious spiral arm structures or dust lanes visible. The general appearance indicates a high degree of central concentration with little to no observed disturbance or merging activity. The overall visual characteristics are consistent with an early-type galaxy.
