The observed galaxy presents as an edge-on spiral, characterized by a prominent central bulge that appears smooth and somewhat boxy. The disk is viewed nearly perfectly edge-on, displaying a distinct elongated shape. There is a relatively uniform distribution of light across the disk, with a gradual decrease in intensity moving away from the central bulge. No distinct spiral arm structures are visible due to the edge-on orientation. The color profile indicates an older stellar population with a concentration of redder hues, particularly within the bulge region, suggestive of evolved stars and a lower rate of ongoing star formation. There appear to be no signs of active galactic nuclei or recent major merger events disturbing the overall morphology.
