The galaxy presents a smooth, elliptical morphology with a notable central bulge. The core region exhibits a high surface brightness, indicating a concentration of stellar mass. The overall shape suggests a relatively low degree of flattening, appearing close to round but with a slight elongation. Light distribution falls off gradually from the center outwards, with no apparent spiral arm structures or distinct features disrupting the smooth profile. There may be some minor disturbances, but nothing to suggest an active major merger. The galaxy appears to be an isolated system, based on its morphology and lack of close companions in the field of view. Colors indicate star formation activity but not intensely high levels.
