The galaxy presents as a relatively compact and smooth object. Its overall shape is elliptical, appearing largely spheroidal with no readily discernible spiral arm structure or bar. The light distribution is centrally concentrated, with a bright, unresolved core that likely corresponds to the galactic nucleus. The color profile is fairly uniform, exhibiting a bluish-white hue, suggesting the presence of at least some young, hot stars contributing to the overall luminosity, but not a high number. There are no obvious signs of recent major merger events. Faint outer regions are discernible, indicative of a stellar halo surrounding the main body of the galaxy. The smoothness of the galaxy indicates that it is a relaxed system that could be forming stars at a moderate rate.
