The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a dominance of older stellar populations, indicated by the yellowish hue concentrated in the central region. There is a subtle color gradient, shifting towards slightly bluer tones in the outer regions, which could indicate the presence of some younger stars or ongoing, but limited, star formation. No distinct spiral arms or other prominent morphological features are readily discernible, giving it a somewhat amorphous and rounded appearance. There appear to be some disturbances in the lower portion of the galaxy, potentially a minor interaction.
