This galaxy exhibits a generally smooth morphology with a concentrated central bulge. The light distribution is largely featureless, with no apparent spiral arms or prominent dust lanes visible. There may be some subtle asymmetries or disturbances in the outer regions, suggesting potential past interactions or minor tidal effects. The galaxy appears approximately round in shape, with a slight elongation along one axis. The color profile suggests an older stellar population, particularly in the central regions, which exhibit a yellowish-orange hue. The outer regions show a hint of bluer light, potentially indicating younger stars, though this is not pronounced. Overall, the galaxy appears to be relatively massive, and the light is quite concentrated.
