The galaxy appears to be an elliptical galaxy, exhibiting a predominantly smooth, spheroidal morphology. There is little evidence of spiral arms or significant disk-like structures. The galaxy presents a centrally concentrated luminosity profile, with brightness gradually decreasing towards the outer edges. The overall shape is largely round, with minimal ellipticity. There is no apparent indication of ongoing major mergers or tidal disturbances, though subtle minor disturbances cannot be definitively ruled out based on the available imagery. The galaxy's color appears to be a relatively uniform blue-green, suggesting a stellar population that may contain some young or hot stars, but a more precise spectral analysis would be required to confirm this. The overall structure suggests an evolved system that has largely completed the process of hierarchical assembly, although subtle features may be present but are unresolved at this image resolution.
