The galaxy appears to be an elliptical galaxy with a smooth, rounded morphology. A slight disturbance or possible tidal feature can be observed near the main galactic body, potentially indicating a past or ongoing interaction with a smaller galaxy or object. The galaxy's core exhibits a bright, concentrated luminosity, suggesting a high density of stars within the central region. The color gradients suggest an older stellar population with a redder hue dominating the central region, while bluer colors appear faintly in the outer regions, indicating a slight presence of younger, hotter stars. The galaxy is relatively compact, with a moderately sized halo of diffuse light extending outwards. The overall structure implies a relatively evolved galaxy, potentially undergoing or having undergone recent merger activity.
