The galaxy presents as an elliptical morphology, exhibiting a generally smooth, featureless appearance with a central bulge. The light distribution is concentrated towards the center, fading gradually outwards. The color profile suggests an older stellar population, with a reddish-yellow hue dominating the galactic structure. There is little evidence of spiral arms or dust lanes. The galaxy appears somewhat elongated, deviating slightly from a perfectly circular shape. There may be some evidence of minor gravitational disturbance, possibly due to a past or ongoing interaction. The overall structure indicates a relatively evolved galaxy, possibly approaching quiescence in terms of star formation.
