The galaxy presents a largely elliptical morphology, exhibiting a high degree of radial symmetry. The light profile appears smooth and centrally concentrated, with a gradual decline in surface brightness outwards from the core. There is no apparent spiral structure or evidence of a prominent disk. The color is moderately red, indicating a population of older stars with lower ongoing star formation. Slight asymmetry is observed suggesting a possible minor disturbance, with a faint extension or tidal feature. Overall, the galaxy is likely a relatively evolved system, with limited current star formation and a significant population of older stars, indicative of an elliptical galaxy type.
