The galaxy presents an overall smooth morphology with a clear central bulge, suggestive of an elliptical or lenticular type. It exhibits a slightly elongated shape, deviating from perfect circularity. The central bulge is characterized by a yellowish hue, likely indicating an older stellar population. Surrounding the bulge, a faint disk-like structure is discernible, displaying a bluer color, potentially indicating younger stars and ongoing star formation. There is no evidence of a significant spiral arm structure or major disturbances in the galaxy's overall shape, suggesting a relatively quiescent state. The smooth appearance and lack of distinct features indicate that this galaxy is not currently undergoing any major merging events. Some minor asymmetry may be present, warranting further investigation into the possibility of minor tidal interactions. The general color profile implies a galaxy with a mixed population of older and younger stars, although the older population appears to dominate the central regions.
