The galaxy presents as a generally smooth object, with an elliptical morphology. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. Proceeding outward, a gradual transition to a blue-green color shift is observed, implying the existence of younger, bluer stars within the surrounding regions. There is an apparent lack of distinct spiral arm structures or significant dust lanes, further supporting its classification as an elliptical galaxy. The overall shape is somewhat elongated, with an intermediate aspect ratio, indicating it is neither perfectly spherical nor highly flattened. There is no indication of a prominent galactic nucleus. Additionally, there is no evidence of major tidal disturbances or ongoing mergers; however, a slight asymmetry might point toward a minor interaction.