The galaxy presents a primarily smooth morphology, with a largely elliptical profile. The main body of the galaxy is concentrated, displaying a yellow-orange hue, indicative of an older stellar population and potentially a lack of significant ongoing star formation. There is a very faint suggestion of minor disturbances present on one side of the galaxy. These disturbances are possibly a tidal feature, suggesting a past or ongoing interaction with another galaxy. Overall, the galaxy's appearance is relatively undisturbed, suggesting that it has been quiescent for a significant period of time. The galaxy has some small features suggesting that it may be in the process of merging or has previously merged with another galaxy.
