The galaxy appears to be a relatively smooth, elliptical or lenticular system. The central bulge is prominent, exhibiting a yellowish hue, suggestive of an older stellar population. A faint disk may be present but is difficult to ascertain, due to the overall smoothness of the galaxy's light distribution. There's no apparent spiral structure, and the galaxy is fairly round in appearance, with a slight elongation. No significant signs of tidal disturbances or ongoing major mergers are visible, although a subtle asymmetry is noticed on the outer parts of the galaxy. The light is concentrated toward the center. The galaxy appears relatively isolated, with no close companions visibly interacting with it.
