The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless with a high degree of central concentration of light. There is little evidence of spiral arms or a distinct disk structure. The galaxy exhibits a yellowish-white hue, suggesting a stellar population dominated by older, redder stars with a relatively low rate of on-going star formation. Its apparent round shape suggests a classification nearing E0 or E1 on the Hubble sequence. Subtle color variations suggest the presence of minor dust lanes or subtle areas of bluer, younger stellar populations, although they are not prominent. No signs of tidal tails or other signs of recent or ongoing major merger activity are observable. The galaxy appears undisturbed and relatively isolated.
