The galaxy presents as a concentrated, elliptical morphology. The light is highly concentrated towards the center, suggesting a prominent bulge. There is a gradual decrease in light intensity moving outward from the core. There is a lack of distinct spiral arms or structures, instead appearing as a relatively smooth distribution of light. There may be an underlying disk structure obscured by the bulge light and the distance to this galaxy. There appears to be some color variation, with a slightly bluer tint to the outer region, and a yellowish-orange color to the concentrated core. There are no indications of major mergers or tidal disturbances from this image. The general morphology suggests a fairly evolved system.
