The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution with a moderate degree of ellipticity. The color profile suggests an older stellar population, with a centrally concentrated yellowish hue indicating a bulge dominated by evolved stars. Fainter bluish halos are present, likely indicating a low level of on-going star formation or the presence of a younger stellar population in the outer regions. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears relatively isolated and undisturbed, showing no signs of recent major merger events, although the presence of some minor disturbance cannot be ruled out.
