The galaxy presents as a relatively smooth, elliptical or lenticular structure. It has a central bulge that appears predominantly yellow, suggesting an older stellar population with less ongoing star formation. The galaxy exhibits a slight elongation, but does not present any distinct spiral arm structures. Faint blueish hues can be seen in its outer regions, which indicates the presence of younger, hotter stars in the surrounding halo. There may be evidence of minor tidal disturbances or interactions with other nearby galaxies, but the overall form appears regular and largely undisturbed.
