The galaxy presents a generally smooth, elliptical morphology. It appears somewhat rounded in shape, with a lack of prominent features such as spiral arms or a distinct central bar. The light profile exhibits a concentration toward the core, with a gradual decrease in intensity outward.

Color analysis suggests the galaxy is relatively red, indicative of an older stellar population and potentially lower rates of on-going star formation. There is a slight color gradient observed between the inner and outer regions. The core appears more yellow/orange, while the outskirts have a slightly bluer hue. This may suggest some recent or ongoing star formation in the outer parts of the galaxy.

There is no obvious evidence of any major mergers or tidal disturbances.
