The galaxy presents as a generally smooth, elliptical-like structure, exhibiting a high degree of radial symmetry. There is a bright, concentrated central bulge that dominates the overall luminosity profile. The luminosity appears to fall off gradually with increasing radius from the core. The color is generally homogenous, with a yellowish-white hue suggestive of an older stellar population. There is no clear indication of significant dust lanes, spiral arms, or other features indicative of ongoing star formation. A very slight elongation is perceptible, though the galaxy appears nearly circular. Evidence of any tidal disturbances or interactions with neighboring galaxies is absent. The galaxy appears to be a relatively undisturbed system.
