The galaxy appears to be a spiral galaxy, although its structure is somewhat distorted and difficult to fully resolve. The central bulge is present but not prominently defined. Some spiral arms can be discerned, but they appear to be disrupted, possibly indicating a recent or ongoing interaction with another galaxy. There is a slight color gradient from the center outwards, with the central region exhibiting a yellower hue, possibly indicative of an older stellar population. The outer regions of the galaxy show bluer patches, suggesting ongoing star formation within. The overall morphology leans towards being somewhat smooth, but there is also evidence of features indicative of a more disturbed state. It seems to be a single object with a hint of interaction with another nearby galaxy.
