The galaxy appears to be a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars and potentially a supermassive black hole at its center. Moving outwards from the core, the light gradually diffuses, forming a soft, extended halo. There is little evidence of significant spiral arm structure or prominent dust lanes within this system. The galaxy is not perfectly circular, leaning more towards being between circular and elliptical. There is no definitive indication of any major ongoing merging events, although there might be a slight asymmetrical feature that could suggest minor tidal disturbances or a past merger event. The galaxy's morphology appears consistent with an older stellar population, indicated by its redder color and the lack of distinct blue star-forming regions.
