This galaxy presents as a moderately sized, elongated, disk-shaped object. The central bulge appears prominent with a concentrated, reddish hue, suggesting an older stellar population likely dominated by red giant stars. The galaxy exhibits a relatively smooth texture, with no sharply defined spiral arm structures readily apparent. There is a subtle color gradient observed from the core outwards, transitioning from a warm orange-red in the center to a more diffuse yellowish-white at the edges, which might imply some recent or ongoing star formation in the outer regions. The overall morphology hints towards an evolved system, potentially a lenticular galaxy or a spiral galaxy with tightly wound arms seen at a relatively high inclination. There appears to be minor disturbances present in the galaxy, but not enough to define it as a major merger.
