The galaxy presents as a concentrated, generally smooth, luminous object. The core is a bright yellow-white, with a comparatively dense structure. There is a noticeable radial decrease in luminosity moving outward from the central bulge. While largely smooth, there are subtle hints of faint, diffuse disc-like structure extending from the core region. There is a very slight blueish tint to the outer regions of the disc. The galaxy exhibits an approximately circular morphology, showing little apparent distortion and is likely an early-type spiral galaxy. There is no obvious indication of a major merger event, though there are very slight disturbances visible. There is an absence of prominent dust lanes or highly defined spiral arms. The star formation rate appears to be suppressed.
