The galaxy appears as a diffuse, somewhat elongated structure with a subtle bluish tint. Its morphology suggests a disk-like form, although lacking prominent spiral arms or a well-defined central bulge. The light distribution is relatively smooth, but some regions within the galaxy seem slightly brighter and more concentrated than others. There might be hints of internal structure, like faint, disrupted arms or irregular star-forming regions. Overall, the galaxy presents a moderately disturbed or possibly merging state, indicating potential ongoing gravitational interactions. It seems relatively small in physical size and does not show evidence of intense star formation activity.
