The galaxy exhibits a generally elliptical morphology, with a high degree of central concentration and a relatively smooth light distribution. The galaxy appears slightly flattened in the image, with a discernible major axis and minor axis. It has a yellowish hue, potentially indicative of an older stellar population with reduced ongoing star formation. There is very little evidence of spiral arm structure or prominent dust lanes. A small amount of blue light can be seen mixed into the yellowish hue of the galaxy, potentially showing on-going star formation at a low level. The overall appearance is consistent with that of an elliptical galaxy undergoing passive evolution.