This galaxy presents as a relatively smooth, centrally concentrated object with a moderate ellipticity. The light distribution suggests a dominant bulge component, potentially classifying it as an early-type spiral or an elliptical galaxy. Faint outer regions extend from the central core, and these appear largely featureless. The color profile indicates a slightly bluer hue at the core with the redness suggesting an older stellar population. There may be signs of minor disturbances or interactions.
