The galaxy presents an overall elliptical morphology, appearing largely smooth with a concentrated central bulge. There is a lack of prominent spiral arm structure or other distinct features typically associated with disk galaxies. A slight elongation is perceptible, but the shape is generally rounded. The color profile suggests a composition of older stellar populations, with a central yellowish hue grading to a bluer color in the outer regions, possibly indicating some ongoing, albeit limited, star formation. No signs of major mergers or significant tidal disturbances are apparent.
