The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is a prominent, concentrated region of light, appearing yellowish, indicating a population of older stars. The galaxy exhibits a moderately high degree of roundness. There's some subtle, diffuse light extending outwards from the core, suggesting the presence of a faint disk or halo component, although distinct spiral arms are not apparent. The overall morphology suggests a system that is not currently undergoing major merging activity, with only some minor internal disturbances.
