The galaxy presents as a flattened, elliptical system, with a smooth, diffuse light distribution. A notable central bulge dominates the overall structure, appearing brighter and more concentrated than the surrounding disk. The color gradient suggests a relatively uniform stellar population, possibly indicating an older stellar population. The absence of well-defined spiral arms or dust lanes is apparent. The galaxy exhibits an apparent rotation, oriented along its major axis. There appears to be no evidence of ongoing major merger activity, nor any distinct tidal features disrupting its overall morphology, instead showing potential minor disturbances. There are no distinct regions of active star formation.