The galaxy presents as a centrally concentrated object with a generally smooth profile. The light distribution suggests an elliptical morphology, appearing moderately elongated, though tending more toward a round shape. There is no clear evidence of spiral arm structure or a distinct disk. The galaxy's central region is brightest and exhibits a yellowish hue, indicating a potentially older stellar population. Fainter, bluer regions appear as patchy extensions along the galaxy's main axis, possibly sites of recent, low-level star formation. The overall structure shows subtle asymmetry, which may be a sign of minor disturbances or gravitational interactions. No major ongoing merger events are readily apparent based on its current morphology.
