The galaxy presents a centrally concentrated luminosity profile. The central region is notably bright, with a predominantly smooth appearance and a slightly elongated morphology. A subtle asymmetry is present, with a possible minor disturbance or faint tidal feature extending from the primary body of the galaxy. The overall color is consistent with an evolved stellar population, but hints of blueish coloration in the outer regions indicate pockets of younger stars may exist. No distinct spiral arm structure is clearly visible. The galaxy appears to be generally undisturbed, with some likelihood of a minor interaction or internal feature disrupting its otherwise smooth shape.
