The galaxy presents a generally smooth and somewhat elongated morphology. Its color profile suggests a dominance of older stellar populations, exhibiting a yellowish-white hue concentrated toward the central bulge. There is a slight color gradient between the core and the outer regions, with the outermost parts appearing subtly bluer, possibly indicating the presence of younger, although relatively subdued, star formation in the galactic disk. No distinct spiral arms or prominent dust lanes are readily apparent. There's a subtle asymmetry in the outer edges of the galaxy, hinting at a potential minor tidal interaction or disturbance.
