This galaxy appears to be relatively compact, displaying a central, luminous region surrounded by a more diffuse halo. The core exhibits a bright, almost unresolved nature, suggesting a concentrated source of luminosity, potentially an active galactic nucleus or a dense stellar population.

Moving outwards from the center, a fainter, asymmetrical structure can be discerned. There's a distinct, elongated feature extending from the main body, possibly indicative of a tidal tail or a disrupted arm due to gravitational interaction. The overall morphology suggests a transition between a smooth elliptical form and a disturbed system, with signs of recent or ongoing interaction. The color gradients indicate varying stellar populations within the galaxy, with bluer colors potentially associated with younger stars and star formation regions.
