The galaxy appears to be an elliptical galaxy, displaying a smooth, diffuse light profile without any prominent spiral arms or distinct disk structure. The central region of the galaxy exhibits a higher concentration of light, indicating a possible bulge component. The galaxy's overall shape is elongated, suggesting a deviation from perfect sphericity, with an apparent cigar-shaped morphology. There is no evidence of any ongoing major merging events or significant tidal disturbances affecting the galaxy's structure. Subtle color variations are observed within the galaxy. The central bulge region appears redder than the outer regions. This might indicate an older stellar population residing within the galactic core. The outer halo exhibits bluer hues.