The galaxy appears as a single, somewhat elongated, amorphous object. There appears to be a central bulge with a diffuse halo. The color of the object indicates a relatively older stellar population; this is supported by the smooth appearance of the galaxy. There is little evidence of spiral arms or dust lanes. The overall structure does not present any clear signs of significant ongoing merging activity, although there may be minor disturbances. The central region shows a slightly brighter, concentrated area, which may indicate the presence of an active galactic nucleus, although this is not definitively discernible from this image alone. The overall shape tends toward being between round and elongated.
