The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated bulge that transitions into a less defined disk. The color gradient suggests a population of older stars, particularly in the bulge. The disk itself shows a subtle blue tinge, which could indicate regions of more recent, albeit limited, star formation. The galaxy shows signs of some tidal disturbance, but is generally undisturbed, indicating a lack of any recent major merging events. The overall shape deviates slightly from a perfect sphere, appearing more elongated or cigar-shaped. The size is intermediate, neither very large nor a dwarf galaxy.
