The galaxy appears to be a spiral galaxy, viewed at a high inclination. The central bulge appears prominent and is a yellow-white color, indicating an older stellar population. The disk of the galaxy is visible as a faint, elongated structure extending from the bulge. The disk exhibits a color gradient, with the regions closer to the bulge appearing more yellow and the outer edges exhibiting a slightly bluer hue, suggesting the presence of younger stars in the spiral arms. The galaxy exhibits signs of a possible interaction or merger. There is a bright, secondary condensation located slightly offset from the main galactic center. The overall form of the galaxy is somewhat disrupted, with the disk showing irregular features rather than a smooth, well-defined structure. There are signs of low rates of star formation.
