The galaxy presents a complex morphology, exhibiting characteristics of both a smooth elliptical structure and a disturbed or merging system. The central region displays a concentrated brightness, possibly indicative of an aging stellar population. Extending outwards from the core, diffuse light suggests a stellar halo. A clumpy, uneven distribution of light in the outer regions possibly indicates ongoing tidal interactions or recent merger events. Some faint, wispy extensions are observable. The overall color suggests a mix of stellar populations, with redder colors dominating the central regions.
