The galaxy exhibits a relatively small angular size. It presents a somewhat irregular morphology. A central, bright core is evident, likely representing a high concentration of stars in the galactic nucleus. Surrounding this core, a fainter, diffuse structure is observed. There are hints of what might be disturbed spiral arms or tidal features, suggesting a possible interaction or past merger event. Based on color, the central region appears to be composed of older stellar populations while the outer regions may contain younger, hotter stars. A lack of distinct features suggests that the galaxy could be an elliptical or lenticular type galaxy with some disturbances.
