The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a bright, yellowish-white hue. There is little indication of significant spiral arm structure or prominent dust lanes. The galaxy appears largely spheroidal, displaying a high degree of roundness in its overall shape. Minor asymmetrical disturbances or tidal features are not readily apparent, indicating a relatively quiescent state with no recent major merger events. The outer regions of the galaxy gradually fade into the background sky, suggesting a lack of ongoing, intense star formation in the disk. The core of the galaxy emits a notably stronger and more concentrated light signal compared to its outer regions.
