The galaxy presents a generally smooth and concentrated morphology. It exhibits a moderately round shape, with a slight deviation from perfect circularity. The light distribution is relatively even across the galaxy's body, with a central region that appears marginally brighter, indicating a possible central bulge or core. There are no prominent spiral arms, bars, or tidal features readily visible. Based on the lack of obvious distortions, there is no significant evidence of ongoing major merger activity. There is also no appearance of significant interaction or presence of a major disturbance occurring. The color of the galaxy appears somewhat redder overall.
