The observed galaxy presents as a flattened, disk-like structure, viewed edge-on. A prominent central bulge is apparent, displaying a yellowish hue, suggesting an older stellar population and/or significant dust obscuration. The disk itself is less luminous and exhibits a bluer color profile compared to the bulge, suggestive of ongoing or recent star formation within the disk. The dust lane is difficult to make out, but is likely present in the equatorial plane. There is no visible evidence of any major mergers or strong tidal interactions. The bulge appears to be round in shape. 
