The galaxy presents an elliptical morphology, appearing largely featureless and smooth in texture. Its color profile indicates a dominant population of older stars, as evidenced by the yellowish-red hue concentrated towards the central bulge. The galaxy exhibits a slight elongation, but is generally consistent with an elliptical classification, with the bulk of its light emanating from the central region, suggesting a high degree of stellar density there. There is faint bluer light on the edges, indicating a small population of younger stars and the possibility of some ongoing, albeit limited, star formation. There are no spiral arm structures or obvious dust lanes are visible. The overall appearance suggests that this is a relatively mature galaxy.
