The observed galaxy presents as a roughly elliptical, disk-like structure with an approximate diameter of 10 units, where units are estimated by the Petro Th50 parameter. The central region exhibits a bright, concentrated luminosity, appearing smooth in texture and white in color. Surrounding this central bright region, a less luminous area is visible, exhibiting a predominantly cyan hue. The outer periphery of the galactic disk displays a complex distribution of color, showing localized regions of red, green and blue, possibly indicating areas of active star formation or dust. The overall light distribution does not indicate a strong spiral arm structure or bar, instead it shows an unstructured disk morphology. There is a slight hint of possible minor disturbance in the symmetry of the disk, specifically a small deviation, suggesting a minor interaction. A significant part of the galaxy shows a smooth and non-distinct feature. There is no indication of a major merger event or a major disturbance.
