The galaxy presents as a somewhat smooth, elliptical structure, with a concentrated central bulge. The light distribution suggests an overall spheroidal shape, though with some elongation visible along a northeast-southwest axis. The galaxy exhibits a distinct color gradient. The central region appears more yellow and orange, potentially indicating an older stellar population with a lower rate of star formation and a higher concentration of dust. Progressing outward from the core, the galaxy displays bluer hues primarily on the Northwest side, hinting at younger, hotter stars and more active star formation occurring in this region, or less dust. A small, moderately bright red point source is visible on the southeast end.
