The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular classification. Its shape is more in between round and cigar-shaped. The central region exhibits a bright, concentrated core, indicative of a significant stellar population and possibly an active galactic nucleus. Moving outward from the core, the galaxy displays a gradual decrease in luminosity, with the outer regions appearing fainter and less defined. There is some evidence of slight disturbance in the structure, but appears generally isolated. The overall color profile tends towards redder hues, possibly indicating an older stellar population with lower rates of ongoing star formation. The estimated size appears moderate for a galaxy at its redshift.
