The galaxy presents as a largely featureless, elliptical-like structure. The light profile suggests a relatively smooth and concentrated distribution, exhibiting a high degree of central light concentration. The galaxy's color appears to be dominated by yellow and green hues, indicating a stellar population that is likely dominated by older, redder stars with possibly some intermediate age stars that are slightly younger and bluer. There is no readily apparent dust lane, spiral arm structure, or significant irregular morphological feature. The morphology is consistent with a relaxed system with very little ongoing star formation and no signs of recent merger activity. The galaxy appears to be isolated with a roughly round shape.
