The galaxy presents a relatively smooth, elliptical morphology. It is generally round in appearance, with a slight deviation towards a cigar shape. The light distribution is fairly uniform across the galaxy, suggesting a well-mixed stellar population. There is no clear evidence of a prominent disk structure or spiral arms, which supports the classification as an elliptical galaxy. No distinct features of an ongoing merger or major tidal disturbance are visibly present, although some minor disturbances may be present. The light is most intense around the core. It's color suggests there is evidence of recent star formation. Overall, it has an estimated stellar mass significantly greater than our Sun. The specific star formation rate is quite low.
