This galaxy appears to be a relatively compact system, exhibiting a generally smooth morphology. While a distinct central bulge is not readily apparent, there are subtle variations in color and intensity across the galaxy's profile. The light distribution appears to be concentrated towards the central regions, suggesting a higher stellar density there. The galaxy displays a slight elongation, deviating from a perfectly circular shape. There are some subtle signs of minor disturbances in its structure, and the galaxy may be interacting with other systems, although there is no clear, ongoing merger.
