The galaxy presents an elliptical morphology, appearing as a smooth, elongated structure. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in surface brightness towards the outer regions. The color profile indicates a generally older stellar population, with a hint of recent star formation activity appearing as slightly bluer regions in the outer disk. The overall shape is moderately elongated. There is a suggestion of minor disturbances. There is no strong evidence of active merging activity.
