The galaxy presents as a concentrated, elliptical object. The central region exhibits a bright, yellowish hue, suggesting a significant population of older stars. Moving outward from the center, the color gradually transitions to a cooler, bluer tone, indicating the presence of younger stars. The galaxy displays a relatively smooth, featureless morphology, with no distinct spiral arms or bar structures visible. The overall shape is somewhat elongated, tending towards an elliptical form, yet not extremely cigar shaped. Some subtle asymmetry is apparent, possibly hinting at minor gravitational interactions or disturbances, though the overall structure is not dominated by strong signs of an ongoing merger. The faintness of the outer regions suggests a low surface brightness.
