The galaxy presents as a somewhat diffuse object. A bright central core region exhibits a high concentration of light, possibly indicative of an active galactic nucleus or a dense stellar population. Surrounding the central region is a fainter, more extended halo or disk-like structure. This structure appears to be somewhat irregular in shape, with hints of non-uniform light distribution, potentially suggesting tidal disturbances or ongoing interactions with another galaxy. The color profile indicates a mix of stellar populations, with the central regions appearing slightly bluer compared to the outer regions, suggesting younger, hotter stars in the core. There are some localized bright spots or knots within the outer structure, which could indicate regions of active star formation or particularly dense stellar clusters. Overall, this galaxy exhibits characteristics of a system that has potentially undergone a recent interaction or merger event.
