The galaxy presents an overall irregular morphology with a central region exhibiting a distinctly blue hue, potentially indicative of active star formation within a relatively dust-poor environment. The outer regions of the galaxy appear more diffuse and exhibit a reddish tint, perhaps suggesting an older stellar population or the presence of dust absorption. There is evidence of a possible weak bar-like structure oriented along a northwest-southeast axis. No well-defined spiral arms are apparent, and the galaxy may be undergoing some form of minor disturbance or merging event based on its irregular form. There is a lack of prominent bulge. The galaxy shows clear evidence of neutral hydrogen. The stellar mass is estimated to be considerable, suggesting that the galaxy is a fairly massive system, despite its lack of a well-defined morphology.
