The galaxy presents as a relatively smooth, rounded structure. There is a notable lack of spiral arm definition or distinct features. The light distribution appears fairly uniform across the galactic disc, suggesting a lack of prominent star-forming regions. The core of the galaxy exhibits a slightly higher intensity of light compared to the outer regions, which are fading. There is a hint of possible minor disturbance in the uniformity of the light distribution, possibly indicating recent or ongoing interactions with a satellite galaxy. However, the overall structure does not indicate signs of a major merger event. The galaxy does not seem to be a irregular shaped object and most likely a spherical shape based on the even light distribution across the surface.
