The galaxy presents a largely smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in luminosity outward. The galaxy exhibits a dominant yellowish hue. The shape is close to round, displaying minimal apparent ellipticity. There is no evidence of spiral arm structure or a prominent disk. There are no obvious signs of recent or ongoing major merger activity or tidal disturbances. The limited color variation suggests a relatively homogenous stellar population throughout the galaxy, likely dominated by older stars. The low rate of current star formation suggests it is a relatively quiescent system. The estimated size is approximately 3 kpc across, placing it within the range of a dwarf or intermediate-mass elliptical galaxy.
