The galaxy appears as a generally smooth, elliptical structure. It exhibits a bright, concentrated central bulge that transitions gradually to a fainter, more diffuse halo. The shape is somewhat elongated, but not excessively so, appearing more oblate than cigar-shaped. The light distribution suggests an older stellar population, with a yellowish-orange hue dominating the color profile. There is no apparent spiral arm structure or prominent dust lanes visible. The overall impression is of a mature galaxy, with a relatively high degree of symmetry and no obvious signs of recent merger activity or significant star formation. The galaxy presents a cohesive and integrated form.
