The galaxy presents as a generally smooth, elongated structure, appearing nearly edge-on from our vantage point. It exhibits a subtle color gradient, with the central regions appearing slightly redder, while the outer edges show a bluer hue. This could suggest the presence of younger, hotter stars in the galactic disk. The overall shape resembles a flattened spheroid, potentially indicative of a spiral galaxy seen from its side, or perhaps an elliptical galaxy with a flattened morphology. There are subtle irregularities in the galaxy's profile. These irregularities suggest potential disturbances or interactions with other galactic structures.
