The galaxy presents as a moderately bright, elliptical morphology. Its core exhibits a concentrated, yellowish-white luminosity, suggesting an older stellar population is likely present. Surrounding the core is a more diffuse, greenish halo. Given the smooth appearance and lack of obvious spiral arm structure, this appears to be a relatively evolved system. There may be some minimal disturbances. The ellipticity of the galaxy is subtle, leaning towards "in-between" classifications, but with the suggestion of a slight elongation along its major axis.
