The galaxy presents an elliptical morphology. The light distribution appears smooth, with no distinct spiral arms or bar structures visible. The central region exhibits a bright, concentrated nucleus, suggesting a potentially active galactic nucleus or a high density of stars. The color gradient transitions smoothly from a yellowish core to a slightly redder outer halo. There is no obvious evidence of recent major merger activity or tidal disturbances in the immediate vicinity. The overall structure suggests a relatively evolved galaxy with a significant population of older stars. Faint disk-like features appear present.
