The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that diffuses outwards, without any prominent spiral arm structures or a significant disk. The light distribution is relatively uniform, with the color indicating an older stellar population, potentially with a low rate of on-going star formation. There is no indication of any tidal tails, obvious mergers, or significant disturbances in the surrounding field of view. The galaxy appears roughly circular. The object is estimated to be at a redshift of approximately 0.2, and it presents an apparent magnitude implying it is a reasonably luminous object at its given distance.
