The galaxy presents an overall elliptical morphology, exhibiting a high degree of central concentration. The light distribution appears relatively smooth, with a gradual decline in intensity from the bright, unresolved core outward. There is a subtle color gradient observed, with a slightly bluer hue in the outer regions compared to the redder central bulge. The lack of prominent spiral arm structures suggests a classification leaning towards an early-type galaxy. There appears to be very faint, minor irregularities in the outer envelope, indicating a possible interaction or minor disturbance event in the past. The object's roundness is notable; deviation from a perfect ellipse is minimal.
