The galaxy presents as a largely smooth, elliptical structure. It exhibits a concentrated central bulge region, emitting primarily in the red-yellow spectrum. This central region gradually diffuses into a fainter halo. There is subtle evidence of possible faint, extended features or shells surrounding the main body of the galaxy. The overall color suggests an older stellar population dominating, with little evidence of significant ongoing star formation. There may be evidence of a minor disturbance in the outer structure of the galaxy, perhaps the beginning of a merger, but this disturbance does not affect the galaxy's core. The round, smooth shape of this galaxy classifies it as elliptical.