This galaxy presents as a relatively compact, flattened system, likely an early-type spiral or lenticular galaxy, though the resolution limits definitive morphological classification. It appears to have a smooth, centrally concentrated bulge. There is evidence of a faint disk component, although the image lacks the clarity to resolve distinct spiral arms. The galaxy appears to be actively forming stars in a small portion of the galaxy, which is an area of great activity in the blue light spectrum. The light distribution suggests that there is no major ongoing merger event, nor do there appear to be significant tidal disturbances.
