This galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. The central region appears brighter and more yellow in color, suggesting a concentration of older stars. The outer regions are less defined, with a more diffuse, bluish glow. This color gradient could indicate ongoing, albeit low, levels of star formation in the outer regions. The overall shape appears roughly circular, with minimal evidence of spiral arms or a distinct disk. There is very little indication of interaction or tidal disruption from other galaxies. It appears to be an isolated system exhibiting properties consistent with an early type galaxy or a transitioning spiral galaxy.