The galaxy presents a generally smooth morphology, with a dominant central bulge. The shape of the galaxy appears to be transitioning from round to elliptical, closer to a disk than a sphere. There may be some minor disturbance in the galaxy's structure, but it is difficult to classify given the resolution. The color gradient suggests the presence of both older stellar populations, indicated by redder hues, and possibly younger, hotter stars, indicated by blue. There is a yellow/orange area on the left side, but overall, this seems to be a singular galaxy instead of a merger between two galaxies.
