The galaxy presents an elliptical morphology, though the precise classification is complicated by observed disturbances. The galaxy's core appears smooth and bright, with a central concentration of luminosity. Extending outwards from the core, a faint disk structure is discernible. The disk appears relatively thin and elongated, suggesting a significant inclination relative to our line of sight.  

The color distribution within the galaxy indicates active star formation, especially toward the center. The presence of redder regions in other areas may indicate older stellar populations or dust obscuration.  

Morphological irregularities are present, suggesting potential recent or ongoing interactions or disturbances.  The asymmetry may indicate past tidal interactions. No distinct spiral arms are resolved in the images.
