The galaxy presents as a luminous, extended object with a generally smooth appearance. Its shape is predominantly elliptical, exhibiting a high degree of sphericity. The color distribution suggests a relatively homogenous stellar population, skewed towards older stars. There are no apparent spiral arms or dust lanes, although a very subtle asymmetry could point to minor disturbances or past interactions. Overall, the galaxy’s morphology is consistent with an elliptical galaxy, likely a substantial system with moderate star formation.
