This galaxy exhibits a fairly compact morphology. There is evidence of a central, brighter region, possibly a galactic bulge or nucleus. Surrounding this central region is a fainter, more diffuse halo. The galaxy does not appear to possess well-defined spiral arms or a clear disk-like structure. There appears to be some degree of asymmetry or irregularity in the outer regions, potentially indicative of tidal interactions or past merger events. A slight elongation is observed in the image. The colors indicate it is emitting in the blue/green part of the spectrum. 
