The galaxy presents a generally smooth morphology, with a bright, concentrated central bulge. It exhibits an elliptical shape, tending toward a more elongated, intermediate form rather than a perfectly circular appearance. There are subtle indications of possible minor disturbances in the outer regions, though no major mergers or strong tidal features are readily apparent. The color profile suggests the presence of older stellar populations, especially within the central bulge, with a gradual shift toward bluer hues in the fainter, more diffuse outer regions, indicative of ongoing, albeit limited, star formation. The overall structure points towards a lenticular or early-type spiral galaxy, viewed at a shallow inclination.
