The galaxy exhibits a primarily smooth morphology with a subtle disk-like structure. Its color profile indicates a central concentration of older stellar populations, seen as a yellowish-orange hue, surrounded by a bluer, somewhat flattened region suggesting the presence of younger stars or ongoing star formation within the disk component. The image shows a possible minor disturbance in the overall symmetry of the galaxy, with a slight asymmetry in the outer regions. A very faint patch of nebulosity or tidal feature is visible near one edge, which could indicate minor interactions or previous merger events. Overall, the galaxy appears to be transitioning between a purely elliptical form and a more structured spiral or lenticular morphology.
