The galaxy presents as a largely elliptical morphology with a smooth profile. The central region exhibits a concentrated luminosity, appearing more yellow in coloration, suggesting an older stellar population. Fainter, somewhat redder regions are visible extending from the core. The object does not display a prominent disk-like structure or spiral arms. There is no obvious evidence of tidal tails or distortions indicative of a recent major merger event, though a minor asymmetry cannot be ruled out. Color gradients across the galaxy's body likely reflect variations in stellar population age and dust content. Overall, the galaxy appears as a relatively evolved system.
