The observed galaxy appears to be a merging system, or potentially a galaxy with a significant tidal disturbance. One component presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated core and a diffuse halo. The second component is more compact, with a slightly irregular morphology that may indicate ongoing interaction. This is a possibility, since the galaxy's colour index from the composite image suggests a redder population in the first, smooth component, and a bluer, possibly younger stellar population in the secondary, more disturbed component. The overall shape is elongated, not perfectly spherical, suggesting an intermediate shape. There may be minor disturbances within the primary component that indicate a previous or ongoing interaction.
