The galaxy presents a largely smooth, elliptical morphology. The light distribution suggests a spheroid-dominated system with a relatively concentrated central region exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions appear fainter and slightly bluer, hinting at the presence of some younger stars or a small amount of ongoing star formation. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy's shape is moderately elongated; between a circle and a cigar shape. There are no obvious signs of a major merger or significant tidal disturbances affecting the galaxy's structure, suggesting that it has not undergone a major interaction recently.
