The galaxy presents a generally smooth, elliptical morphology. The central region exhibits high luminosity, appearing bright and concentrated. Moving outwards from the core, the light gradually decreases. There is little indication of spiral arms or significant dust lanes within the galaxy's structure. The overall shape is fairly circular. There is no evidence of any major disturbances or ongoing merger activity affecting the galaxy's morphology. The color indices, inferred from the red, green and blue image data, suggest an older stellar population.
