The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The light distribution appears relatively smooth throughout, lacking prominent spiral arms or distinct features associated with active star formation in the outer regions. A slight colour gradient is observable, trending from a bluer hue at the core to a redder, yellowish halo extending outwards, possibly indicating an older stellar population in the galaxy's outskirts. There are indications of some dust, but it is evenly distributed, not obscuring any particular region of the galaxy. The object appears relatively isolated, showing no major signs of gravitational interaction or ongoing mergers with other galaxies. There is evidence of a central bar feature bisecting the galaxy. Overall, based on its morphology, the galaxy is best classified as a lenticular galaxy, possibly an early-type spiral galaxy.
