The galaxy presents as a moderately bright elliptical or lenticular type, exhibiting a relatively smooth and centrally concentrated light profile. Its overall shape is somewhat elongated, with a noticeable, but not extreme, ellipticity. There is a diffuse halo extending beyond the central bulge. There is no evident spiral arm structure or dust lane obscuration. The color appears generally redder, suggesting an older stellar population. The morphology indicates a system that has likely undergone significant dynamical evolution, potentially through mergers or interactions, resulting in a homogenized stellar distribution and reduced star formation activity. The presence of a faint halo further supports this history. The surface brightness appears to diminish gradually from the center, characteristic of a galaxy with a well-established spheroid component.
