The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical in shape, exhibiting a high degree of roundness as opposed to a more elongated or disk-like structure. There is no apparent presence of spiral arms or a distinct disk component visible in this image. The light profile decreases gradually from the core outwards, with no clear signs of ongoing major merging activity or tidal disturbances. The color is a yellowish hue, potentially indicating a population of older stars, and little active star formation.
