The galaxy presents as an elliptical or lenticular structure, exhibiting a relatively smooth and diffuse appearance without well-defined spiral arms. Its overall shape is slightly elongated. The central region is noticeably brighter and more concentrated, suggesting a prominent galactic nucleus or bulge. There's a subtle color gradient visible, with the central region appearing more yellowish-white and the outer edges displaying a hint of bluer tones. This may indicate a difference in stellar populations, with older stars concentrated towards the center and younger stars or ongoing star formation occurring at the periphery. There is no strong evidence of recent or major merging events, though there could be minor disturbances. The overall structure is reasonably smooth. The estimated size is around 6 kpc. The observed colors indicate a moderate redshift.
