The galaxy presents as a centrally concentrated object. Its morphology appears to be generally smooth, with a high degree of ellipticity. The core exhibits a bright, concentrated region, surrounded by a more diffuse halo. There are minimal signs of spiral arm structure or prominent dust lanes. The color profile suggests a population of older stars, with a redder hue dominating the overall appearance, although there is evidence of some bluer light emanating from the central region. There may be minor disturbances due to interactions with other objects or recent accretion events, but the primary structure remains relatively undisturbed.
