The galaxy presents as a somewhat elliptical structure, with an intermediate axis ratio, neither distinctly circular nor highly elongated. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms or significant dust lanes. The dominant color is a yellow-orange hue, which could indicate a population of older stars and a relatively low rate of on-going star formation. There is a suggestion of tidal disturbance or potential ongoing merger activity in the form of faint diffuse extensions.
