The galaxy presents a predominantly smooth and elliptical morphology. It displays a concentrated central bulge that emits light primarily in the yellow spectrum, which might indicate an older stellar population. Surrounding the bulge, a more diffuse halo extends outward, exhibiting a bluer tinge suggesting ongoing or recent star formation activity, albeit at a low rate. A subtle, minor disturbance appears on one side of the galaxy, possibly hinting at a previous interaction or merger. Overall, the galaxy appears as an intermediate, moderately massive system exhibiting characteristics of an evolving, yet largely quiescent, galaxy.
