The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated light profile. Its overall shape is largely spheroidal, although some slight elongation may be present. A core component appears to be contributing to the galaxy's overall luminosity. The galaxy displays a faint disk-like structure that shows some disturbance in its shape. There are minor morphological disturbances that indicate a non-negligible interaction or minor merger history.&#x20;
