The galaxy presents as a generally smooth, centrally concentrated object with a slightly elliptical morphology. It exhibits a bright, yellowish core region, surrounded by a more diffuse, fainter halo of light. Faint hints of blue are visible around the edges, possibly indicating regions of younger, hotter stars. No distinct spiral arm structures or strong dust lanes are apparent. There is little evidence of recent major merger activity or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed. Its overall structure suggests a relatively evolved system, possibly an elliptical or lenticular galaxy viewed at a substantial distance, with a moderate amount of star formation occurring within the galactic boundaries.
