The galaxy appears to be a relatively compact, elliptical system. Its overall shape is spheroidal, showing a smooth and largely featureless light distribution. There is a concentration of light towards the center, suggesting a prominent galactic nucleus. The color profile indicates a general reddening from the central region outwards, implying an older stellar population in the outer regions and potentially younger, bluer stars closer to the core. There is some evidence of a slight asymmetry or minor perturbation in the light distribution, which might be indicative of a past interaction or minor merger event. While the main body of the galaxy is smooth, subtle irregularities or faint extensions cannot be ruled out at this resolution.
