The galaxy appears as an elongated structure with a relatively smooth overall appearance. Its shape is somewhat cigar-like, but not extremely so; it could be described as transitional between round and elongated. The central region exhibits a brighter, more concentrated light, suggesting a bulge or core component.

Fainter, somewhat irregular extensions are visible extending from the central region, indicating a possible disk-like structure. Patches of bluer light are interspersed within this disk, suggestive of some ongoing, albeit subdued, star formation. These blue regions are not particularly prominent, implying that star formation is not vigorous.

There's also some indication of a possible minor disturbance in the galaxy's morphology, potentially related to past interaction with another galaxy, although it is subtle. There isn't any obvious, major ongoing merger activity, just perhaps a small companion or tidal feature.

Overall, the galaxy presents as a relatively low-mass, quiescent system with a hint of past interaction and a moderate degree of smoothness.
