The galaxy presents a largely smooth, elliptical morphology. Its overall form is notably rounded, exhibiting little deviation from a circular shape. The central region displays a concentrated, bright core with a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy exhibit a fainter, blueish halo, which may indicate the presence of younger stars or a small degree of ongoing star formation. There are no readily discernible features such as spiral arms or a distinct disk structure. The galaxy appears relatively isolated, showing no significant signs of tidal disturbances or ongoing merging activity with other galaxies. 
