This galaxy presents a predominantly smooth and elliptical morphology. There is little evidence of prominent spiral arms or a well-defined disk structure. The light distribution appears centrally concentrated, gradually fading towards the outer regions. The galaxy exhibits a color gradient, transitioning from a bluer hue in the core to slightly redder tones in the outskirts. This might indicate an older stellar population dominating the outer regions, with potentially ongoing or recent star formation more concentrated toward the center. There are subtle irregularities in the isophotes but generally, the shape is regular. Faint extensions or tidal features are not readily apparent, indicating a lack of recent major merger events.
