The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated, bright central region, indicative of a significant stellar population. The galaxy displays a yellowish hue in its core, which may suggest an older stellar population, with relatively little ongoing star formation. There is a subtle color gradient outward from the core, with the outer regions appearing slightly bluer. The overall symmetry suggests that the galaxy is relatively undisturbed, and does not appear to be undergoing a major merger. There is minimal evidence of spiral arm structure or dust lanes. Small chance of some minor disturbance, possibly a small interaction, but mostly uneventful history. The size appears to be moderately large, indicating it is a fairly large galaxy.
