The galaxy exhibits a smooth, elliptical morphology, appearing mostly featureless. The central region displays a concentrated bulge, with a yellowish hue indicative of an older stellar population. This core gradually fades into a disk-like structure, though distinct spiral arms are absent. The galaxy's overall shape is somewhere between round and elongated. The color gradient suggests a lack of significant ongoing star formation. There are no signs of major disturbances or ongoing merger events. It appears to be an isolated galaxy, and the features are indicative of a gravitationally relaxed system.
