The galaxy presents as a primarily smooth structure, exhibiting a concentrated central bulge that dominates the overall light profile. The bulge appears almost spheroidal and lacks any discernible fine structure at this resolution. A faint, extended disk component surrounds the bulge, although its spiral arm structure, if present, is not clearly resolved. The disk's color seems to be somewhat bluer than the bulge, suggesting the presence of a younger stellar population in the disk. The galaxy's overall shape appears somewhat elongated. There is a hint of a very minor disturbance of some kind, but nothing that indicates an active merger. Overall, the galaxy gives the impression of being an intermediate system between a pure elliptical and a spiral, potentially a lenticular type.
