The galaxy appears as an elliptical morphology, with a smooth, featureless light distribution. The galaxy's shape is elongated, exhibiting a cigar-like appearance. A concentration of light towards the center suggests a prominent bulge. The color gradient indicates a redder core with possibly older stellar populations, transitioning towards slightly bluer hues in the outer regions, hinting at the presence of younger stars although significantly less. There are no visible signs of spiral arms, tidal tails, or active galactic nuclei. The galaxy does not appear to be undergoing any major mergers or significant disturbances.