The galaxy presents as an elliptical morphology, appearing smooth and largely featureless. The color profile suggests an older stellar population, with a concentration of light toward the redder end of the spectrum, indicating evolved stars. There's a notable absence of discernible spiral arms or significant dust lanes. The light distribution is centrally concentrated with a gradual decline in brightness moving outward. There may be a slight flattening, with the galaxy appearing closer to spheroidal, but some ellipticity is seen. No major or minor disturbances are apparent and there are no signs of any ongoing merger events.
