The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. It appears approximately circular in shape. The core region exhibits a bright, yellowish-white luminosity, suggestive of an older stellar population. A faint greenish hue surrounds the core, potentially indicative of ongoing, low-level star formation activity. There is no clear evidence of spiral arm structure or a prominent disk. A very slight asymmetry is detected in the outer regions of the galaxy, but no obvious signs of a major ongoing merger are visible. The overall appearance is consistent with an early-type galaxy, likely an elliptical or lenticular system. The estimated size and luminosity of the galaxy place it within the range of a typical dwarf galaxy, yet its high mass indicates it may have already undergone substantial stellar evolution.
