The galaxy presents as a centrally concentrated elliptical morphology, appearing largely smooth and featureless. The core exhibits a bright, yellowish hue, suggesting a population of older stars. A faint, diffuse halo of light extends outward, transitioning to a reddish color. There are no visible spiral arms or dust lanes. The overall roundness suggests a classification towards E0 or E1 on the Hubble sequence, though the color profile indicates potential ongoing, albeit low, star formation. There is no visual evidence of any major merging activity or tidal disturbances.
