The galaxy presents as a somewhat face-on spiral, appearing disk-like. A bulge is visible, concentrated towards the galaxy's center, exhibiting a yellowish-white color, suggesting an older stellar population in this region. The galaxy displays a fairly uniform structure, with a dominant disk and a spiral arm visible at its lower left. This arm shows a concentration of blue-ish light, indicative of ongoing star formation activity.

There is evidence of morphological disturbance within the galaxy, as the spiral arms are not clearly defined and exhibit an irregular structure. There also seems to be a possible tidal tail or merging component emanating from the left side of the disk. The galaxy's color gradients suggest an ongoing star formation process, more active in the disk region compared to the bulge. The overall shape indicates a system undergoing, or having recently undergone, some form of interaction. The inferred mass suggests that this is likely a galaxy. HI Measurements suggest the presence of neutral hydrogen gas.
