The galaxy presents as an elongated, spindle-shaped structure, suggestive of a disk galaxy viewed at a significant angle. There is a notable color gradient, with a concentrated, yellowish-white core that likely represents an older stellar population within the galactic bulge. Fainter, bluish hues are visible extending outward from the central region along the major axis, indicating the presence of younger, hotter stars possibly residing within spiral arm structures. These arms appear diffuse and not well-defined, giving the galaxy a somewhat smoothed appearance. There are no obvious signs of recent major mergers or strong tidal disturbances in the immediate vicinity, though minor irregularities in the outer regions cannot be ruled out based on the image quality. Overall, the galaxy exhibits characteristics consistent with a late-type spiral galaxy or possibly a lenticular galaxy with ongoing, albeit modest, star formation in its disk.
