The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer regions. There is little indication of spiral arms or other distinct structural features. The core exhibits a yellowish hue, suggesting an older stellar population. Fainter blue colors appear in the outer regions, suggesting some ongoing star formation activity. Overall, the galaxy shows slight asymmetry, with subtle disturbances, but no major signs of active merging.
