The galaxy presents a largely featureless, smooth morphology. Its overall form appears to be elliptical, with a high degree of central concentration. The luminosity profile suggests a centrally bright region fading smoothly outwards. Color gradients are subtle, exhibiting a slightly yellower central region suggestive of an older stellar population, with bluer tints towards the outer edges. There is no apparent spiral structure, bar, or prominent dust lane obscuration. Minor asymmetry is present, and there may be some slight disturbance in the galaxy's shape, such as potential tidal features, but these disturbances appear minimal. There are no clear signs of ongoing major merging activity. Star formation appears to be relatively suppressed.
