The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. There is a noticeable central bulge that is bright and concentrated with light, possibly indicative of an older stellar population. The luminosity gradually decreases from the center outwards. The overall shape is somewhat elongated, though not exceptionally so. There is a hint of bluer light in the outer regions, which may suggest some ongoing star formation, although it is not the dominant feature. No prominent spiral arms or dust lanes are readily apparent.
