The galaxy appears to be a faint, somewhat diffuse object. Its morphology is not clearly defined; it lacks a distinct spiral arm structure or a well-defined elliptical shape. There is a suggestion of some minor disturbances in its structure, perhaps indicating interaction with another galaxy or past merger events. The central region seems slightly more concentrated, but not to the degree that would classify it as a strong bulge. The overall color is suggestive of a mixed stellar population, with some evidence of both older, redder stars and younger, bluer stars. It is difficult to determine with certainty whether it is primarily a disk galaxy seen at an oblique angle, or a more irregular or dwarf galaxy.
