The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It has a moderate ellipticity, appearing somewhat elongated, with a slight flattening. The core region exhibits a yellowish hue, likely indicating an older stellar population. The outer regions of the galaxy fade gradually into the background, with a bluer tinge that suggests the presence of younger stars or ongoing star formation at a low level. No distinct spiral arms or dust lanes are visible. There might be a minor disturbance visible, but it doesn't appear to be undergoing a major merger. The galaxy appears fairly isolated.