The object appears to be a lenticular or elliptical galaxy, presenting a smooth, elongated profile. The core exhibits a concentrated, brighter region, likely the galactic nucleus. Moving outwards from the core, the luminosity gradually decreases. There is a discernible color gradient, with the central bulge appearing more yellow or orange. This suggests an older stellar population, predominantly composed of evolved stars. The outer regions are fainter and bluer, indicative of some degree of ongoing or recent star formation, although the overall star formation rate appears relatively low. The galaxy lacks a clear spiral arm structure or significant dust lanes. Its overall morphology suggests a system that has largely exhausted its gas supply, leading to a decline in star formation activity. There is no evidence of major mergers or tidal disturbances in the image.
