The galaxy presents a generally smooth, elongated morphology, indicating it may be an elliptical or lenticular type. Its light profile appears centrally concentrated with a diffuse, fading edge. There seems to be an extension of the galaxy that is likely a part of the same galactic system. It has a hint of blue color suggesting some ongoing star formation activity. The main body of the galaxy presents colors that trend toward a redder spectrum, characteristic of older stellar populations. No prominent spiral arms are visible. The object is most likely in a stage where any spiral arms that may have been present in the past have begun to dissolve. The overall structure suggests a galaxy that has either completed or is nearing the completion of a transformation from a spiral to elliptical type, possibly due to a recent minor merger or interaction.
