The galaxy appears to be a lenticular or early-type spiral galaxy, displaying a generally smooth morphology with little evidence of active star formation in the visible bands. The object exhibits a central bulge that is fairly prominent and appears mostly featureless, contributing significantly to the galaxy's overall luminosity. A hint of a disk component might be present, indicated by a slight elongation and the presence of fainter, diffuse light extending outwards from the bulge. The galaxy's color suggests a population of older stars, consistent with its low star formation rate. There's no clear evidence of spiral arms or ongoing mergers, implying that the galaxy is relatively undisturbed. The roundness of the galaxy suggests a moderate inclination relative to our line of sight.
