The galaxy exhibits a complex morphology, indicative of an ongoing or recent merger event. The primary component appears as a spheroid with a concentrated, bright core. Diffuse light emanates outward from the core, though no distinct spiral arm structure is visible. A secondary, smaller structure is observed extending from the primary spheroid. This secondary structure has a more elongated shape and exhibits a distinct color gradient, transitioning from a redder hue near the primary component to a bluer tint at its furthest extent. This structure also shows signs of tidal distortion. The galaxy overall is relatively compact. There appears to be some irregularities that may be dust or star forming regions within the merging system. The smooth fraction of the galaxy suggests that is likely disturbed. Overall this galaxy has a redshift which would suggest that it is significantly distant from the Milky Way.
