The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a relatively uniform stellar population, with a notable absence of distinct spiral arms or significant dust lanes. The overall shape deviates slightly from perfectly round, exhibiting a mild elongation suggestive of an E4-E5 classification on the elliptical scale. There's no obvious evidence of any recent major merger events, although a slight asymmetry in the outer halo region cannot be ruled out as a minor disturbance. The color is generally yellowish, suggesting a population of older, redder stars dominating the light output.
