The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless structure. The central region displays a higher surface brightness, suggesting a concentration of older stellar populations. The overall color profile leans towards redder hues, indicative of an evolved stellar population with a lower rate of ongoing star formation. The shape is elongated, with a major axis estimated around 5 kiloparsecs. There is no apparent evidence of spiral arms, bar structures, or active galactic nucleus activity based on this image alone. There are no obvious signs of tidal disturbances or interactions with neighboring galaxies. The galaxy appears generally isolated and undisturbed.
