The galaxy presents as a luminous, somewhat spheroidal object exhibiting a yellowish hue, indicative of an older stellar population. There is a noticeable structure comprised of two distinct components or nuclei. The primary, more prominent component is brighter and appears relatively smooth in texture. The secondary component is less luminous, with a similar color profile but smaller in apparent size. 

There are indications of tidal distortions or interactions. The galaxy shows evidence of ongoing or recent merging activity, suggested by its irregular shape and the presence of two nuclei. While the overall morphology is relatively smooth, subtle disturbances in its light distribution are seen, giving it a more complex structure. It is unclear if the color variation across the galaxy indicates differing levels of star formation.
