The galaxy presents as a slightly elongated spheroid, with a smooth, relatively featureless appearance. The central region exhibits a concentrated brightness, suggesting a prominent galactic nucleus. The overall color profile leans toward the redder end of the spectrum, hinting at an older stellar population. There is a lack of readily discernible spiral arm structure or dust lanes. The morphology suggests an elliptical galaxy, potentially experiencing relatively low levels of recent star formation activity. Faint color variations may indicate some ongoing, albeit subdued, star formation or localized variations in metallicity within the galaxy.
