The galaxy appears as a centrally concentrated object, exhibiting a dominant spheroidal component. There is a notable absence of distinct spiral arm structures, with only subtle color variations in the outer regions that may indicate areas of low-level star formation. The galaxy is largely smooth in texture, with a fairly symmetrical structure. The galaxy's shape could be described as somewhat elliptical. There is no prominent central bulge, but rather a gradual increase in luminosity toward the core. Overall, the galaxy seems to be relatively isolated, with no obvious signs of ongoing tidal interactions or major mergers.
