This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. The central bulge exhibits a bright, concentrated luminosity profile, suggesting a high stellar density in that region. Moving outward from the core, the luminosity gradually decreases.

The galaxy's overall shape is somewhat elliptical, though close to round. There is no clear indication of spiral arms or a well-defined disk structure. Faint, diffuse extensions of light are visible, which may be stellar halos, tidal features, or the result of minor gravitational interactions. There is no indication of major mergers. Color gradients are subtle, with the central regions appearing slightly more yellow than the outer regions, which display a bluer hue.

The inferred stellar mass indicates that this galaxy is of intermediate size. Its current star formation rate appears to be low.
