The galaxy presents an overall smooth morphology, appearing as an elliptical or lenticular type based on its lack of distinct spiral arms. The central region exhibits a high concentration of light, suggesting a prominent bulge. The light is mostly yellow, indicating a population of older stars. The galaxy appears somewhat flattened, hinting at the presence of a disk component even though distinct features are not visible. There is no apparent ongoing major merger activity. Subtle disturbances might be present, but they are not readily visible.
