The galaxy presents a generally smooth and elliptical morphology. It appears well-defined, with a concentrated central region that gradually fades into its outer regions, suggesting a lack of distinct spiral arms or significant substructure. The galaxy exhibits a yellowish hue in its core, possibly indicative of an older stellar population. Fainter, diffuse blue light surrounds the central region, suggesting the presence of some younger, hotter stars but with a low star formation rate. The overall symmetry and lack of visible distortions suggest the galaxy is relatively undisturbed, without any major ongoing merger events. It appears to be a single, relatively isolated system.
