The galaxy appears as a relatively smooth object with a slight central concentration of light. The overall morphology suggests an elliptical galaxy or a lenticular galaxy seen at a shallow inclination. There is a hint of a disk-like structure, although it is not sharply defined. The galaxy exhibits a yellowish hue, indicative of an older stellar population. No distinct spiral arms or prominent dust lanes are visible. There are no clear signs of a major ongoing merger, although some minor disturbances in the galaxy's shape cannot be entirely ruled out, but the lack of tidal tails or strong asymmetries suggests that it is not a recent merger. The galaxy is moderately luminous, appearing somewhat brighter in redder wavelengths. The light is relatively uniform, with no obvious bright knots of star formation. It is a galaxy with a considerable mass and low ongoing star formation.
