The galaxy presents as a flattened spheroid, displaying an intermediate ellipticity. A central bulge region exhibits a concentrated, bright, yellowish-orange hue, suggesting an older stellar population. Emanating outwards from the bulge, a faint, bluish-green disk structure is visible, indicative of ongoing star formation. This galactic disk appears relatively smooth, lacking prominent spiral arm structures. The galaxy's overall color index indicates a mix of stellar populations, with a greater presence of older stars in the bulge and younger stars in the disk. There is a hint of a slight disturbance or asymmetry in the outer disk, possibly suggesting a minor interaction or past merger event, but it is predominantly a single, isolated galaxy. The overall morphology suggests a transitionary state between an elliptical and a spiral galaxy.
