The galaxy presents as a centrally concentrated system with a generally smooth, elliptical morphology. The light distribution suggests a bulge-dominated structure, appearing more luminous and reddish towards the core, indicative of an older stellar population. The outer regions exhibit a fainter, more diffuse glow with a slight greenish hue, potentially indicating the presence of some younger stars or ionized gas, though star formation appears minimal. There is a noticeable absence of distinct spiral arms or prominent dust lanes. The galaxy's overall shape suggests a classification along the lines of an elliptical galaxy, possibly of type E3-E5, exhibiting moderate ellipticity. There is no visual evidence of any major ongoing merger events or significant tidal disturbances, however, some very minor disturbances cannot be ruled out.
