The galaxy presents as a centrally concentrated, relatively smooth object. The morphology is predominantly elliptical in nature, with a high degree of central luminosity. The color profile suggests an older stellar population with an overall yellow to reddish hue, though the disk has a light blue color. There's no visible spiral arm structure, suggesting a classification towards the S0 end of the Hubble sequence, if not a fully developed elliptical. There is no evident dust lane obscuration, and no apparent ongoing major merger events or tidal distortions. There may be some minor asymmetry that warrants further investigation into whether this could be a minor disturbance. The shape appears generally rounded with an approximate physical size of approximately 2 kpc across its radius. The galaxy appears quiescent in terms of star formation. 
