The galaxy presents an elliptical morphology, with a smooth light distribution. Its overall shape is elongated, exhibiting an axis ratio suggestive of an E4 or E5 classification on the Hubble sequence, where E0 is perfectly circular and E7 is the most elongated. No distinct spiral arms or bar structures are discernible. The core region appears brighter and more concentrated than the outer regions, which gradually fade into the background sky. The color profile indicates a yellowish-white hue, possibly indicative of an older stellar population with relatively low ongoing star formation. No obvious signs of recent major merger events, tidal tails, or strong dust lanes are apparent. Subtle disturbances cannot be ruled out given the image resolution.
