The galaxy presents as a highly elongated structure, suggesting an edge-on disk orientation relative to our line of sight. A central bulge is apparent, exhibiting a relatively smooth, concentrated luminosity profile. The galaxy's color distribution indicates a radial gradient, with the central region appearing more luminous and exhibiting a yellowish hue, potentially indicative of an older stellar population or dust obscuration. The outer regions of the disk appear fainter and slightly bluer, suggestive of ongoing star formation, although the color difference is subtle. There is no immediately apparent presence of spiral arms, which may be due to the edge-on view. The overall morphology suggests that it is likely a disk galaxy with a significant bulge.