This galaxy presents as an elliptical-like structure, though a subtle disk component may be present. The overall shape is somewhat elongated, approaching a cigar shape. The central bulge exhibits a notable concentration of light, appearing relatively smooth and lacking in distinct features. Fainter, bluer regions appear toward the outer edges of the galaxy, suggesting pockets of star formation are present, with an estimated stellar mass on the order of 10^10 solar masses. The galaxy exhibits a red shift, indicative of recessional velocity. There is no obvious evidence of any major mergers or significant tidal disturbances. Based on color and morphology, the galaxy is likely undergoing a modest level of star formation.