The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The core exhibits a concentrated, brighter luminosity, transitioning outward to a fainter, diffuse halo. The color profile indicates a redder core, possibly indicative of an older stellar population, with a slight shift towards bluer hues in the outer regions, potentially signaling younger stars. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There may be a very slight asymmetry to the galaxy's shape, but that is likely due to the low resolution of the image. It seems the disk of the galaxy is oriented roughly edge-on to our line of sight.
