The galaxy presents as a luminous, elliptical-shaped structure. Its light profile is characterized by a smooth, centrally concentrated bulge region exhibiting a yellowish hue, suggesting an older stellar population. Extending outwards from the core, the galaxy displays a fainter, more diffuse halo with subtle color gradients shifting toward cooler tones. There is little evidence of spiral arms or significant dust lanes, pointing to a relatively quiescent morphology. The overall appearance is that of a galaxy undergoing little active star formation. The shape appears to be elongated with an axial ratio possibly close to two-thirds.
