The galaxy appears to be an elliptical galaxy, characterized by a smooth, symmetrical, and relatively featureless appearance. The light distribution suggests a spheroidal shape, with a concentration of luminosity towards the center. The color is predominantly yellowish-orange, indicative of an older stellar population dominated by red giant stars. There is little to no evidence of spiral arms or dust lanes typically associated with younger, star-forming galaxies. The smooth light profile and color suggest minimal ongoing star formation and a significant population of older stars. There might be a slight asymmetry or minor perturbation in the light distribution, suggesting a past or ongoing interaction with a smaller galaxy or gravitational disturbance.
