The galaxy presents a largely smooth morphology. It exhibits a generally elliptical shape with a bright, concentrated central bulge that appears yellowish in color, possibly indicating an older stellar population. The surrounding halo is more diffuse and bluish, suggesting the presence of some younger, hotter stars, but the overall star formation rate appears relatively subdued. There is no clear evidence of spiral arm structure or significant dust lanes. A possible slight asymmetry exists in the outer regions of the galaxy, but no major disturbances or merging events are immediately apparent. The galaxy is moderately massive.
