The galaxy presents as an elongated structure, consistent with an edge-on disk galaxy. A prominent bulge is visible, exhibiting a rounded morphology. The disk appears relatively smooth, with little evidence of distinct spiral arms or significant star formation regions. There is no indication of tidal tails, asymmetries, or other morphological features that would suggest a recent major merger. The lack of clear star formation regions and the smooth disk suggests a relatively low specific star formation rate. The galaxy is generally smooth and uniform, with no visible disturbances. The reddish color indicates a population dominated by older stars.
