The galaxy presents a somewhat ambiguous morphology in this imaging. It has a diffuse, yellowish hue suggesting an older stellar population. The general form exhibits a spheroid shape, potentially indicative of an elliptical galaxy. However, there appears to be a slight flattening or extension along one axis. This may denote a disk component, or simply the result of tidal forces or gravitational interactions. There may be a hint of disturbance to the edges of the light profile which could be signs of a past or ongoing merger event. There is no clear spiral arm structure visible. Any further morphological classification would require deeper, higher-resolution imaging.
