The galaxy presents as a single, smooth object with a moderate red-yellow hue. It appears roughly elliptical or spheroidal in shape with a fairly uniform color distribution, suggesting an older stellar population and minimal ongoing star formation. There is evidence of a close companion or significant tidal distortion, indicating a possible merging event. The morphology is generally undisturbed, with a high degree of central concentration. There is no sign of any dust lanes or spiral arm structures. The luminosity is bright, suggesting it is a massive galaxy.
