The galaxy presents a generally smooth morphology, with a dominant central bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. There is a hint of a faint disk structure, though it is not sharply defined. The overall shape of the galaxy appears to be close to round. There is no obvious evidence of a major ongoing merger, although some subtle irregularities could suggest minor tidal disturbances. The galaxy appears to be relatively quiescent in terms of star formation activity.
