The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The galaxy exhibits a slightly elongated shape, suggesting a minor deviation from a perfect circular structure. The core region is noticeably bright, with a yellow-orange hue indicating a population of older stars. There appears to be little evidence of spiral arms or significant dust lanes. Overall, the galaxy presents a consistent color profile with subtle changes in tint from yellow to a more muted yellow with slight red tint towards its edges. The general appearance suggests an evolved system with limited ongoing star formation.
