The galaxy presents a relatively smooth and compact morphology. It is elliptical in shape, appearing more oblong than perfectly spherical, but not significantly elongated. There is a noticeable color gradient from the core to the outer regions. The central region exhibits a reddish hue, suggesting an older stellar population with less ongoing star formation. Moving outwards, a transition towards greenish-yellow tones is observed, potentially indicative of a younger stellar population and/or the presence of ionized gas. No distinct spiral arms or prominent dust lanes are visible, further supporting the classification as an elliptical galaxy. There is little evidence of any major merger events or significant tidal disturbances.
