The observed galaxy presents as an edge-on spiral galaxy. The central bulge is prominent, exhibiting a smooth, rounded morphology, indicative of an older stellar population. A distinct disk is visible, appearing highly flattened and oriented nearly parallel to the line of sight. There is no evidence of ongoing major mergers or significant tidal disturbances. The galaxy has a redder color indicative of little to no current star formation. There is some indication of the presence of dust in the plane of the disk, though no distinct dust lanes are clearly visible. The general morphology and color suggest that the galaxy is composed mostly of older stars.
