The galaxy presents a primarily smooth morphology, suggesting a classification leaning towards elliptical or lenticular. There is a subtle disk feature visible within a larger smooth halo. The galaxy's shape is generally round, exhibiting slight elongation. No signs of major mergers or significant tidal disturbances are visually apparent. A smooth central bulge is present, with evidence of ongoing star formation in the disk. The color gradient suggests an older stellar population dominating the core, surrounded by younger, bluer stars in the outer regions. The system exhibits an intermediate level of star formation activity. Overall, the system appears stable and relatively undisturbed.
