The galaxy presents as a relatively smooth object, with a discernible, elongated shape. Its central region exhibits a concentration of light, appearing brighter and with a yellowish hue, likely indicating an older stellar population. Fainter, somewhat blueish light is observed at the edges of the galaxy; this indicates a more active stellar population. The observed morphology suggests the galaxy does not have a classical spiral or barred spiral structure. No apparent tidal tails or significant morphological disturbances are visible, implying no recent major merger events. The galaxy appears to be an elliptical galaxy.
