The galaxy appears as a single, centrally concentrated object, with a generally smooth morphology. It exhibits a spheroid shape, with a high degree of roundness. The galaxy appears to have little to no apparent disk structure. A dominant central bulge is evident, indicated by a concentrated luminosity gradient. Fainter, diffuse light extends outwards from the central region, diminishing with radial distance. There is no clear evidence of spiral arms or bar structure. There are slight color variations visible within the galaxy, with a more yellow hue in the central regions, and hints of blue along the outer regions of the galaxy. There does not appear to be any major merging, though there appears to be minor disturbances in the surrounding areas.
