The galaxy appears as a somewhat smooth, centrally concentrated object. It exhibits an elliptical morphology with an apparent slight elongation. The light profile gradually fades from a bright central core outwards. There is minimal evidence of spiral arm structure or distinct features. The color appears predominantly composed of intermediate to redder wavelengths, indicating an older stellar population. There is no obvious presence of active star formation. The galaxy does not display signs of significant tidal disturbance or ongoing merger activity, though there may be some minor irregularities present. Overall, the galaxy is likely a relatively quiescent elliptical galaxy with a low star formation rate and a substantial mass.
