This galaxy appears as a relatively smooth, elliptical-like object, exhibiting an overall orange-yellow hue. This color suggests an older stellar population with a lower rate of ongoing star formation. The galaxy appears to be undergoing some disturbance. A merging event may be the cause of the disturbance, or it may be a projection effect.

The galaxy's size is compact. While the image resolution is limited, the morphology appears predominantly smooth, with a high central concentration of light. There is no clear evidence of spiral arms, a prominent disk, or substantial dust lanes.
