The galaxy presents as a moderately luminous object with a generally elliptical morphology. Its light profile appears relatively smooth, with no obvious spiral arm structures or strong dust lanes visible in this image. There is a slight elongation, suggesting that it may not be perfectly spherical. The color is primarily red-shifted, indicating an older stellar population with fewer young, blue stars. Hints of fainter, bluer regions are present, indicating some ongoing star formation. The overall appearance indicates a galaxy transitioning from a spiral to an elliptical morphology, possibly due to interactions or mergers. There is possible merging activity within the galaxy.
