The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth light distribution. A bright, prominent bulge dominates the central region, surrounded by a fainter, elongated halo. The color of the central bulge appears to be yellowish, possibly indicating an older stellar population. The halo exhibits a slightly bluer hue, suggesting the presence of younger stars. The galaxy's shape is not perfectly circular, displaying a moderate ellipticity. There is no visual evidence of spiral arms, bars, or strong dust lanes. The overall impression is that of a relatively undisturbed system, without significant tidal features or signs of ongoing mergers.
