The galaxy appears to be a relatively smooth, elliptical or lenticular system, exhibiting a centrally concentrated brightness profile. Its light is somewhat homogenous with no obvious spiral arm structures or significant dust lanes visible, which suggest an older stellar population. There is a slight elongation observed, but the aspect ratio is close to unity, indicating a near face-on orientation. The galaxy's color indices suggest a higher abundance of older stars as opposed to younger, bluer stars. There is a slightly redder halo, suggesting that the light has been redshifted. The galaxy is fairly isolated with no obvious signs of recent major merger events.