This galaxy presents a relatively smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in luminosity outwards. There appears to be a lack of distinct spiral arm structures or prominent dust lanes. The color profile exhibits a subtle gradient, transitioning from a slightly bluer core to a redder halo. There is no obvious indication of recent major merger events. There is a subtle asymmetry suggesting possible minor interaction or disturbance. The galaxy is moderately bright, and appears to be a typical galaxy in the local universe.
