The galaxy presents as a largely amorphous structure with a bright, concentrated central region. The luminosity falls off gradually from the core, exhibiting a diffuse halo. The overall shape appears somewhat rounded, though subtle irregularities suggest potential tidal disturbances or interactions. The color gradient indicates a population of older stars dominating the central bulge, which transitions to a more complex mix of stellar populations in the outer regions. There is evidence of on-going star formation, likely resulting from minor disturbances. There may be a hint of a faint disk-like component, but the smoothness suggests a lack of significant spiral structure. The morphology points to an elliptical galaxy that is experiencing or has recently experienced a minor interaction.
