The galaxy presents as an elongated object, likely a spiral viewed edge-on. A prominent bulge is visible, exhibiting a concentrated brightness that suggests a high stellar density. Extending outwards from the bulge is a disk, although its structure is not clearly resolved.

There is a possible dust lane bisecting the galaxy along its major axis, though this is difficult to confirm definitively given the image resolution. The color appears somewhat redder within the galaxy than what would be expected without dust, potentially indicating significant obscuration.

The galaxy does not appear to be currently undergoing any major merging activity or tidal disruption. The lack of strong color gradients or clumpy star formation suggests a relatively quiescent state in its star formation history.
