The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a spheroidal morphology, lacking any prominent spiral arm structures or a well-defined disk. The light profile suggests a smooth transition from the bright central region to the fainter outer halo. There's a slight elongation visible, but overall the galaxy approximates a circular shape. The color index suggests the presence of a somewhat older stellar population, with a yellowish-orange hue dominating the galaxy's light, possibly indicating a lower rate of current star formation and a higher proportion of evolved stars. There's no strong visual evidence of ongoing mergers or tidal disturbances. The galaxy appears to be relatively isolated and undisturbed.
