The galaxy presents as a diffuse, centrally concentrated object with an apparent diameter of approximately 3 arcseconds. It exhibits a generally elliptical morphology, with the luminosity profile appearing relatively smooth throughout the main body of the galaxy. The central region of the galaxy is notably brighter and bluer than the outer regions, suggesting a higher concentration of younger, hotter stars or possibly an active galactic nucleus. There is some asymmetry, with a slight elongation or extension visible along one axis, which could indicate a minor tidal interaction or internal disturbance. The overall color is a composite of blue and red light, suggesting a mix of stellar populations. There is a hint of some disturbance in the edges, but no large spiral arms or bar structure can be observed.
