The observed galaxy presents an elliptical morphology, characterized by a smooth and featureless light distribution. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish-white, concentrated core to a slightly redder, fainter halo. The elongation suggests it is likely an E4-E5 type galaxy. There is little to no evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively isolated, showing no signs of major interactions or mergers with other galaxies. Faint tidal features may be present. Overall, the galaxy appears to be a massive, evolved system with a high stellar mass.