The galaxy appears as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. Moving outwards from the core, the light gradually fades, transitioning to a bluish-white tint in the outer regions, which could indicate the presence of younger stellar populations. The overall shape is primarily smooth and featureless, with no obvious spiral arms or distinct dust lanes visible. The galaxy doesn't appear to be undergoing any major merging events or tidal disruptions, although slight disturbances might be present, as seen from some asymmetry in the light distribution. There's a gradual falloff in surface brightness from the core to the edge of the galaxy. The galaxy's color profile suggests that star formation is likely suppressed, relative to a more active spiral galaxy. The galaxy has an estimated size of a few kiloparsecs, which is within the normal range for galaxies of this type.
