The galaxy presents as an elongated, disk-like structure with a noticeable bulge in the central region. The light distribution suggests a relatively smooth morphology, though subtle asymmetries may be present. The color gradient across the galaxy indicates possible variations in stellar populations, with bluer hues towards the outer edges potentially signifying regions of active star formation, and redder tones towards the center possibly indicating an older stellar population. The galaxy appears isolated, showing no obvious signs of major interactions or mergers with other galaxies, although there is some evidence of tidal stretching, possibly from a smaller merger. Based on its morphology, this galaxy is likely a spiral galaxy viewed edge-on.
