The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge that diminishes gradually outward. The light distribution appears fairly uniform without any prominent spiral arm structures or well-defined dust lanes. Overall, the galaxy seems to be mostly homogenous without significant irregularities in its shape, though there seems to be a faint and small secondary source near the main galaxy, suggesting a small possibility of minor gravitational disturbance. The galaxy color index appears to be moderately red overall, suggesting an older stellar population.
