This galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, relatively uniform emission profile in the observed optical bands. There is a noticeable falloff in luminosity moving radially outward from the central region, with a slight elongation or distortion visible in the outer isophotes. This suggests a possible departure from a perfectly elliptical shape. The color gradient is subtle, with the core potentially appearing bluer compared to the slightly redder and fainter outer regions. Subtle disturbances are possibly suggested by the deviation from being perfectly round. Overall, the galaxy is a prominent, centrally-concentrated system with potential signs of morphological peculiarities.
