The galaxy presents a smooth, elliptical morphology. The central bulge exhibits a concentrated luminosity profile, appearing as a bright, nearly spherical structure. There is a color gradient visible; the core exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by red giant stars. Towards the outer regions of the galaxy, the color shifts slightly towards bluer tones, potentially indicating the presence of a younger, albeit small, population of stars. There is no clear evidence of spiral arms or a well-defined disk component. The overall structure appears relaxed and undisturbed, consistent with a lack of recent major merger events, although there seems to be a companion nearby. The effective radius seems relatively small, suggesting a compact galaxy structure, and based on its color, star formation is likely very low.
