The galaxy presents as a flattened, elliptical form with a noticeable central bulge. A smooth distribution of light is observed, transitioning from a bright core to fainter outer regions. The color profile suggests a relatively evolved stellar population, with a yellow-red hue dominating, indicative of older stars. There is a subtle hint of a possible disk-like structure or spiral arms, but the overall smoothness of the light distribution suggests a classification leaning towards an early-type galaxy with a disk. No prominent dust lanes or active star-forming regions are clearly discernible from this image. There appears to be a slight warp in the lower section of the galaxy. The general morphology seems undisturbed with no signs of active merging or tidal features, which could indicate a gravitationally stable system.
