The galaxy appears as a smooth, elongated structure, suggesting an elliptical morphology. Its central region exhibits a higher concentration of light, fading gradually toward the edges. The color profile indicates a population of older stars with a redder hue concentrated toward the center. There is a lack of distinct spiral arm structures or prominent dust lanes. The overall symmetry is largely undisturbed, with no immediately apparent signs of major ongoing mergers or tidal disruptions, though some minor disturbances cannot be ruled out. The cigar-like shape suggests a prolate spheroid structure. The blueish color in the outer portions could indicate some low-level star formation regions.
