The galaxy presents a generally smooth, elliptical morphology. It appears relatively compact, exhibiting a bright, concentrated central bulge that dominates the overall light profile. There is a suggestion of a disk component, but the disk is faint and not well-defined; the light emanating from the disk is significantly less intense compared to the bulge. The color index suggests a redder overall stellar population, with a gradual color gradient from the core outwards. There is no obvious evidence of significant dust lanes or recent major merger activity. Minor tidal features may be present, but they are not immediately obvious in this image.
