The observed galaxy presents as a relatively small, edge-on spiral. The central bulge appears luminous, exhibiting a concentrated, yellow-orange hue, which is suggestive of an older stellar population with minimal ongoing star formation. The galactic disk is highly inclined relative to our line of sight, obscuring detailed spiral arm structure. The disk is comparatively fainter and bluer, indicating the presence of younger, hotter stars within the spiral arms, though this effect is limited. Dust lanes are likely present within the disk, contributing to the observed obscuration and color variations. There is no obvious evidence of a recent major merger or significant tidal disturbance. The overall morphology is consistent with a quiescent spiral galaxy undergoing moderate star formation activity.