The galaxy presents as a centrally concentrated, likely elliptical or lenticular, structure. It appears to be a relatively smooth galaxy with a mostly spheroidal shape, exhibiting a high degree of central symmetry. The color profile suggests a dominant older stellar population, indicated by its yellowish-orange hue. There may be a faint, diffuse outer halo surrounding the brighter central region, although the depth of the image makes definitive assessment challenging. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively isolated, with no obvious signs of major interactions or ongoing mergers. There are subtle indications of minor disturbances, but it is unclear if they are intrinsic to the galaxy itself or due to artifacts.
