The galaxy presents a generally smooth morphology, with minimal discernible substructure. Its shape approximates a circular form, exhibiting high degree of roundness with little deviation towards elongation. The dominant color appears to be a yellow/orange hue, possibly indicating a population of older stars and/or significant dust obscuration. There are suggestions of a faint greenish emission emanating from the outer regions, which may indicate the presence of ionized gas or regions of ongoing star formation, but is most likely noise. No obvious signs of tidal features, merging activity, or significant disturbances are apparent. The galaxy appears relatively isolated, lacking any nearby companions or indications of ongoing interactions.
