The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge which appears to be the brightest region. The overall color profile seems to indicate an older stellar population, trending towards the redder end of the spectrum, with a likely low rate of current star formation. The shape is mostly rounded, with only the slightest deviation from circularity. There is no apparent evidence of any major ongoing merger events or significant tidal disturbances in its immediate morphology.
