This galaxy appears to be a spiral galaxy, although its detailed structure is somewhat obscured, possibly due to distance or dust. The galaxy exhibits a faint, extended disk with a brighter central bulge. Indications of spiral arms are present but poorly defined. There may be some level of disturbance present in the morphology. The core appears slightly asymmetrical and may show signs of a recent or ongoing interaction with a smaller system or the tail end of a larger system interaction. The color distribution suggests older stellar populations with an overall redder hue, implying a relatively low rate of current star formation. However, there are slight tinges of green and blue which may point to some star forming regions.
