This galaxy exhibits a clear disk morphology, with a central bulge and a faint, extended halo. The disk appears to be inclined somewhat edge-on. There is evidence of internal structure within the disk, as it is not uniformly smooth, suggestive of spiral arms or dust lanes that are not well defined at this resolution. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk is bluer in color overall, potentially indicating ongoing star formation. There are no obvious signs of major mergers or significant tidal disturbances.
