The galaxy presents as a generally smooth, elliptical morphology. There is a concentrated central bulge exhibiting a yellow-orange hue, suggesting a population of older stars. The outer regions of the galaxy appear fainter and somewhat more diffuse. The object is largely undisturbed, showing no strong signs of recent major merger activity, though there may be hints of slight asymmetry or minor disturbances in the fainter outer regions. The overall shape tends to a roundness, though not perfectly so. The absence of prominent spiral arms or distinct disk-like features is notable, as is the lack of bright, blue star-forming regions.
