The galaxy presents as a highly inclined disk galaxy, appearing nearly edge-on from our perspective. It exhibits a moderately bright central bulge that appears smooth and spheroidal, with no clear substructure visible. The disk component appears thin and elongated, consistent with a high inclination angle. The overall color of the galaxy is notably redder, particularly toward the central bulge. The red color suggests an older stellar population, lower star formation rate, and potentially higher dust content. No distinct spiral arm structure is discernible. Faint extensions are visible from the disk, likely tidal in nature. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or significant tidal interactions. The smooth appearance of the bulge and disk suggests a galaxy that has experienced a period of relative quiescence following the major formation and early evolution phases.
