The galaxy presents as a lenticular or possibly an elliptical galaxy, exhibiting a moderately elongated shape. It appears relatively smooth in texture with a bright, concentrated central bulge. There is little evidence of spiral arm structure or prominent dust lanes. Color gradients are visible, with the central bulge displaying a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy are comparatively bluer, indicative of some ongoing, though potentially limited, star formation. There is no indication of a major ongoing merger or significant tidal disturbance, but a very minor asymmetry is noticeable in the galaxy's outer structure.
