The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated with a gradual decrease in luminosity moving outward from the core. There is minimal evidence of distinct structural features such as spiral arms or a prominent disk. The galaxy exhibits a spheroidal shape, with a high degree of roundness. No significant tidal distortions or indications of ongoing merger activity are readily apparent. Color gradients suggest a population of older stars, particularly concentrated in the central bulge. The faint outer regions indicate some low-level star formation is still possible. The galaxy appears to be relatively isolated.
