The galaxy presents as a somewhat elliptical structure, with a brighter, concentrated central region. The overall shape exhibits a moderate degree of elongation. The light distribution appears relatively smooth, suggesting a dominant spheroid component. There is a slight indication of a possible disk or arm-like feature extending from the central region. The color of the galaxy appears to be slightly bluer near the extremities, becoming progressively redder towards the core. The galaxy shows little to no evidence of major disturbances or ongoing merging events.
