The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated, displaying a bright, unresolved core that suggests the possible presence of an active galactic nucleus or a dense stellar population. The galaxy appears to be largely featureless, lacking prominent spiral arms or distinct dust lanes. There may be a hint of a disk, but it is very subtle. A blue tint to the light suggests some star formation activity may be occurring within the galaxy. The galaxy appears somewhat spheroidal, with a hint of elongation. No major signs of recent mergers or tidal disturbances are apparent.
