The galaxy presents a moderately elliptical morphology, appearing largely smooth with a subtle central concentration of light. There's a suggestion of a faint, extended halo surrounding the core. The color profile indicates a higher proportion of older stellar populations, with a redder overall hue. There are minor features or disturbances, such as tidal tails or asymmetries, suggesting no recent major merger events or intense star formation. The galaxy is likely a passively evolving system or an early-type galaxy.
