The galaxy presents a somewhat smooth, elliptical morphology with a slight asymmetry. The core exhibits a concentrated, bright, yellowish-orange hue, suggesting a population of older stars. There is a faint, diffuse halo surrounding the core, appearing slightly elongated. A subtle disk-like structure may exist. There is no indication of strong spiral arms or active star formation regions within this structure. There is no apparent merging or major disturbances in the image.
