The galaxy appears to be an elliptical type, exhibiting a smooth, spheroidal morphology. The light distribution is highly concentrated towards the center, displaying a bright, yellowish core indicative of an older stellar population. There is a lack of discernible spiral arm structure or dust lanes, suggesting a relatively quiescent galaxy with little ongoing star formation. The overall color is consistent with a passively evolving system. The galaxy exhibits a generally rounded appearance, with no major distortions indicative of recent mergers. There may be slight disturbances or interactions, but they are not overtly apparent in the provided image.
