The galaxy appears to be a relatively compact system, likely at a considerable distance given its apparent size. The primary body of the galaxy exhibits a smooth, centrally concentrated light profile, suggesting a possible elliptical morphology or a bulge-dominated spiral with a faint disk. Its color is generally green/yellow, indicating the presence of intermediate-age stellar populations. 

There appears to be a secondary component, slightly offset and less luminous, possibly indicating a minor interaction or recent merger event. This secondary component exhibits a bluer hue, suggestive of younger stars or ongoing star formation. The system as a whole does not present with any obvious tidal tails or other signs of major disruption, but a degree of asymmetry can be observed. A faint disk may be present, but not clearly visible. The overall morphology appears intermediate between elliptical and spiral.
