The galaxy presents as a luminous object with an overall morphology somewhere between smooth and having distinct features. The central region exhibits a bright, concentrated core with a yellowish hue, suggestive of an older stellar population. Surrounding this core, a fainter, bluish halo is visible, potentially indicating a younger population of stars or ongoing star formation within a disk-like structure. The galaxy appears generally rounded, with no significant elongation or tidal features immediately apparent, although there may be some minor disturbances. The color gradient from the core to the outer regions indicates spatial variations in stellar populations.
