The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge appears bright and concentrated, with a yellowish hue, suggesting an older stellar population. A disk is implied, though poorly defined, exhibiting a subtle color gradient, transitioning towards slightly bluer tones at the edges. This may indicate the presence of some younger stars towards the periphery, though overall, star formation appears limited. The galaxy is elongated, and the isophotes display some degree of flattening. There is no indication of any major spiral arm structure or significant dust lanes. The overall appearance is consistent with an early-type galaxy, possibly a lenticular galaxy, observed at a slight angle.
