The galaxy appears to be of intermediate size, exhibiting a generally elliptical morphology. The central region presents a high degree of luminosity, indicating a concentrated stellar population or potentially an active galactic nucleus. Moving outward, the luminosity gradually decreases, suggesting a diminishing stellar density with radial distance. While a smooth structure is apparent, subtle irregularities or faint tidal features may be present in the outskirts of the galaxy, potentially hinting at past or ongoing interactions. The overall color profile suggests a mix of stellar populations, with a somewhat redder core implying a greater abundance of older, cooler stars, and bluer outer regions.
