The galaxy appears to be a relatively luminous, early-type system, possibly an elliptical or lenticular galaxy. It exhibits a smooth, concentrated light profile, with a bright, yellowish core that fades into a more diffuse, extended halo. The overall shape is somewhat elongated, but lacks any distinct spiral arm structure or prominent dust lanes. There is a suggestion of a faint, flattened disk component viewed nearly edge-on. No significant tidal features or signs of recent major mergers are evident, although a subtle asymmetry or minor disturbance in the outer regions cannot be ruled out. The color indices suggest that it is dominated by an older stellar population, with low levels of ongoing star formation.
