The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated. There is a slight elongation, suggesting it is somewhere between a perfectly circular and cigar shape. A small amount of bluer emission extends outwards in a disk-like manner. The central region exhibits a brighter, more concentrated luminosity, likely indicative of an older stellar population. There is evidence of some minor disturbance along the outskirts of the galaxy, possibly due to interaction with a satellite galaxy. Overall, the galaxy appears to be a relatively massive system with a moderate amount of ongoing star formation.
