The galaxy presents as a somewhat elongated, though generally rounded, structure. Its light profile appears relatively smooth, with a concentration of intensity towards the center, suggesting a bulge-dominated morphology. There is a slight asymmetry in the outer regions, perhaps due to a minor gravitational interaction. The color indices indicate a population of older stars, evidenced by its redder hues, though there are subtle variations in color across the galaxy, which may be areas of modest star formation. No prominent spiral arms or distinct features are visible, but there is evidence of some irregularity in the overall structure.
