The galaxy presents as a relatively smooth, single structure. There is a concentrated central bulge exhibiting a yellowish-orange hue, which likely indicates an older stellar population and reduced ongoing star formation activity.  The main body appears largely elliptical in shape, with a hint of a disk. It displays an intermediate axial ratio, suggesting a deviation from being perfectly circular but not significantly elongated. Overall the galaxy does not appear to show any major disturbances from mergers. There may be a minor disturbance. No distinct spiral arms are visible. The galaxy displays a slight red shift. The galaxy spans roughly 3.6 kpc across its half-light radius.
