The galaxy presents a largely smooth morphology, with a somewhat elliptical shape. It displays a central, brighter region indicative of a galactic bulge. The galaxy exhibits a yellow-orange hue, possibly indicating an older stellar population and lower rates of star formation. There are some subtle disturbances in the galactic structure, which may point to minor gravitational interactions or past merger events. The galaxy appears relatively isolated, although there are some faint objects in the vicinity that may be interacting with it. Overall, it seems to be an intermediate mass galaxy, currently in a relatively quiescent state.
