The galaxy presents a predominantly smooth morphology, appearing as a well-defined elliptical or lenticular structure. Its shape is generally round, exhibiting minimal deviation from circular symmetry. There is no discernible evidence of spiral arms or a prominent disk. The light distribution is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. The galaxy exhibits a yellowish hue, suggesting a population of older stars, with minimal evidence of ongoing star formation. Overall, the galaxy appears to be relatively undisturbed, with no visible signs of major mergers or significant tidal interactions. The estimated size is approximately 4 kpc.
