The galaxy presents a largely smooth morphology, appearing elliptical in shape. The light distribution suggests a centrally concentrated spheroid, with luminosity decreasing gradually towards the outer regions. The galaxy exhibits a color gradient, trending from redder hues towards the central region to greener hues in the extended halo. The overall color suggests a stellar population that may be dominated by older stars, although some ongoing or recent star formation is not ruled out, as is suggested by the green color in the halo. There is a slight asymmetry to the light distribution that hints at a minor disturbance in the galaxy's gravitational environment. No prominent spiral arms or well-defined dust lanes are evident in the galaxy's structure.
