The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be an early-type galaxy with a high degree of central concentration. There is a very slight deviation from perfect roundness. No prominent spiral arms or disk features are discernible. There's no visual evidence of any significant ongoing merging events or major disturbances in the galaxy's morphology, though there may be minor disturbances. Based on the colors, the galaxy shows evidence of moderate star formation with an appreciable redder color. This suggests the presence of a substantial population of older stars, but with a non-negligible number of younger stars.
