The galaxy presents as a centrally concentrated, relatively smooth elliptical or lenticular morphology. The light distribution is generally symmetric with a slightly elongated shape. There is a notable color gradient, with a distinct reddish or yellowish hue concentrated in the core, suggesting an older stellar population. The outer regions exhibit a bluer color, though these are less prominent. There is no evident spiral arm structure or significant dust lane obscuration. The galaxy appears to be relatively isolated, showing no major signs of tidal disturbance or ongoing merger activity. The light profile appears smooth, indicating a lack of significant recent star formation.
