The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. The object exhibits a high degree of radial symmetry, with no apparent spiral arms or distinct features. Its overall shape is round, lacking any significant elongation. There are no visible signs of ongoing major merger activity or significant tidal disturbances. The galaxy exhibits a yellowish-red hue, suggesting a population of older stars and a low rate of star formation. Based on the overall characteristics, this object is most likely an early-type galaxy with little to no ongoing star formation.
