The galaxy appears as a centrally concentrated, luminous object. Its overall morphology is smooth and relatively featureless. There is a significant central bulge exhibiting a high degree of roundness. There is little indication of spiral arms or a well-defined disk structure. The galaxy exhibits a radial gradient in luminosity, with the core being significantly brighter than the outer regions. There is no clear indication of any ongoing major merger activity or significant tidal disturbances. The observed color suggests a population of older stars, with a relatively low rate of star formation.
