The galaxy exhibits a smooth, elliptical morphology, appearing largely featureless without prominent spiral arms or a distinct disk structure. The light distribution is centrally concentrated, with a bright, well-defined core that gradually decreases in intensity towards the outer regions. The shape is slightly elongated with an apparent ellipticity. The galaxy displays a color gradient, with a yellowish-white hue in the central regions, suggesting an older stellar population, transitioning to a slightly bluer, though subdued, color in the outer regions implying the possible presence of younger stars. There are no apparent signs of ongoing major mergers or tidal disturbances.
