The galaxy appears as a centrally concentrated, ellipsoidal structure. Its light profile is smooth with no obvious spiral arm features or dust lanes visible at this resolution. The core of the galaxy presents with a brighter, yellowish-orange hue. This central bulge transitions into a fainter, greenish-blue halo. The ellipticity suggests it is not a face-on disk galaxy but rather an elliptical galaxy or a disk galaxy viewed at an angle. There are no apparent signs of tidal disturbances or ongoing mergers, suggesting a relatively settled morphology. The overall color index appears to be relatively redder. This hints at an older stellar population, and thus a low star formation rate.