The galaxy appears as a relatively smooth, centrally concentrated object with a notable lack of discernible spiral arms or a prominent disk structure. Its overall shape approximates a spheroid, exhibiting a high degree of circularity. The galaxy's light distribution is dominated by a central bulge that fades gradually towards the outer regions. The color of the galaxy suggests a population of older stars, with a yellowish hue predominating. There are no strong indications of ongoing major star formation activity or significant dust lanes, which are common features in spiral galaxies. There may be some hints of minor disturbances in the surrounding halo. Overall, the galaxy appears consistent with an elliptical type, likely at a substantial cosmological distance, exhibiting a mature stellar population and minimal star formation.
