The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a primarily yellow/orange hue, suggestive of an older stellar population. While the image resolution is limited, there is no clear evidence of significant spiral arm structure or active star-forming regions. The overall appearance indicates a spheroid-dominated system, possibly with a low star formation rate. The roundness indicates that the galaxy is not seen edge-on. Some slight disturbances can be seen, perhaps indicating past or current gravitational interactions with another galaxy.
