The galaxy presents as a relatively smooth, elliptical structure. It appears largely spheroidal in shape, with a high degree of central concentration. The color profile is generally uniform, exhibiting a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of on-going star formation. No distinct spiral arms or features are apparent, but a very faint, diffuse disk-like structure may be present. There is no evidence of any major mergers or tidal disturbances.
