The galaxy presents an overall elliptical morphology, appearing mostly smooth and relatively featureless. Its light profile suggests a high degree of central concentration. The core exhibits a yellowish hue, indicative of an older stellar population. A subtle gradient from this core radiates outwards, transitioning into a bluer, less concentrated outer region, suggesting a component of younger stars or ongoing star formation, albeit at a moderate level. Faint, subtle disturbances or irregularities are detectable in the outer disk, potentially signaling past minor interactions or mergers. The galaxy exhibits a slight elongation but is generally rounded in appearance, with no evidence of a prominent disk structure or spiral arms.
