The galaxy presents as a smooth, centrally concentrated object, displaying an elliptical morphology. The central region appears brighter, with a noticeable concentration of light. The overall color profile suggests an older stellar population, with a tendency toward redder hues in the central bulge. There is a faint, extended halo of light surrounding the main body, gradually fading into the background. No distinct spiral arms or prominent dust lanes are discernible. There is very slight distortion of the overall elliptical shape.
