The galaxy presents as an edge-on disk galaxy with a prominent central bulge. The bulge appears to be of a spheroid shape, with a color gradient suggesting a concentration of older stellar populations towards its center. The disk component is visibly flattened and extends significantly beyond the bulge, exhibiting a relatively smooth texture with minimal discernible spiral arm structure. Light from the disk indicates a mixture of stellar populations, with some regions displaying a bluer hue, suggestive of ongoing star formation, particularly towards the outer edges. The high inclination prevents detailed observation of internal features within the disk. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or tidal distortions.
