The galaxy presents a largely smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a flattened, elongated shape, with an axis ratio indicating a moderate degree of ellipticity. The central region appears brighter and more concentrated, with a gradual decrease in luminosity towards the outer regions. There are some subtle color gradients noticeable, transitioning from a yellowish-white core to slightly bluer hues in the surrounding regions. No prominent spiral arms, bars, or other distinct features are readily apparent, indicating a lack of significant ongoing star formation in a highly organized manner. The overall structure suggests an older stellar population dominating the light output. No strong signs of interaction or recent merger events are detected based on visual inspection.
