The galaxy appears to be a relatively smooth, centrally concentrated object. It presents a largely elliptical morphology, exhibiting a high degree of roundness. There is a bright central bulge that diffuses outward with no distinct spiral arm features evident. The galaxy appears to be relatively isolated with no signs of major disturbances or tidal interactions with neighboring galaxies, indicating a quiescent evolutionary state. Color gradients suggest a redder core possibly indicating an older stellar population, surrounded by a bluer, younger population. The overall faintness suggests a significant distance.
