The galaxy presents as a fairly smooth, elliptical-like structure, exhibiting a high degree of central concentration. It appears largely featureless, lacking prominent spiral arms or obvious dust lanes. The overall color gradient indicates a population dominated by older stars, with a yellowish-orange hue concentrated towards the center. The outer regions seem slightly bluer, potentially indicating a small population of younger stars, although this is not a dominant feature. The galaxy exhibits a roughly circular morphology with a hint of elongation along one axis. There is no evidence of major merging activity or significant tidal disturbances in the immediate vicinity. Any star forming regions may be faint and not visually distinct.
