The galaxy presents an elliptical morphology, with a smooth, concentrated central bulge. The light is dominated by yellow and orange hues, indicative of an older stellar population. The outer regions of the galaxy display a gradual fading in luminosity, with little indication of resolved spiral arms or prominent star-forming regions. There is a subtle flattening of the galaxy along one axis, transitioning into a more cigar-like shape. Evidence of minor disturbances are visible, suggesting that it is possibly interacting or merging with a smaller galactic body. Overall, the galaxy's visual characteristics align with a classification toward the elliptical end of the Hubble sequence, exhibiting evolved stellar populations and a smooth, symmetric light distribution.
