The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a spheroidal shape. A concentrated central bulge is present, decreasing in luminosity further from the center. The galaxy does not show any prominent spiral arms or disk-like structures. There is a slight deviation from perfect roundness. No signs of major disturbances such as tidal tails or obvious signs of a recent major merger are detected. Given the color profile, there appears to be a weak but non-negligible level of star formation occurring within the galaxy.
