The galaxy presents as a relatively compact object, exhibiting an overall elliptical morphology. The central region displays a high surface brightness, appearing smooth and almost uniformly illuminated. A faint, extended halo is suggested, but is likely disrupted. The color distribution appears somewhat complex. The core is notably bluer, potentially indicating active star formation or a prominent active galactic nucleus. The outer regions show a transition to a redder hue, possibly indicative of an older stellar population or increased dust obscuration. There is evidence of minor tidal features, such as faint plumes or distortions in the outer regions, suggesting a potential past or ongoing interaction with another galaxy. However, no companion galaxy is readily apparent in the immediate vicinity. The primary light distribution is roughly contained within an area with a radius of approximately two arcseconds.
