The galaxy presents as an elliptical-like structure, exhibiting a central bulge that appears luminous and concentrated, suggesting a high density of older stellar populations. The overall morphology of the galaxy indicates a relatively smooth structure, with a slight deviation from perfect sphericity, approaching a more intermediate elliptical form. There's a disk shape to the galaxy, as well as an area of disruption that is consistent with a tidal tail, suggesting a history of interaction with another galaxy. There is not a strong spiral pattern, but rather an area of disturbance that is indicative of a minor merger, possibly due to another galaxy. Given the redder hues concentrated within the central region, the dominant stellar population is likely composed of older, evolved stars. The faint bluish tendrils extending from the central region could indicate regions of younger star formation, although limited. There is little to no dust apparent, which is consistent with the classification of an elliptical galaxy.
