This galaxy presents a moderately elliptical morphology, appearing somewhat elongated along its major axis. Its color profile suggests a composition of older stellar populations, with a yellowish-white central bulge dominating the overall light emission. Hints of bluer regions are visible in the surrounding disk, indicating the presence of younger, hotter stars and ongoing star formation, though at a relatively low rate. There is a subtle asymmetry present in the disk. No clear spiral arm structures are resolvable. The galaxy is relatively isolated, with no immediate signs of major tidal interactions or ongoing mergers. The galaxy appears to be a typical example of a transitioning galaxy, experiencing only a limited amount of star formation. 
